Post–T Tauri Stars in the Nearest OB Association
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We present results of a spectroscopic survey of X-ray– and proper-motion–selected samples of late-type stars in the Lower Centaurus–Crux (LCC) and Upper Centaurus–Lupus (UCL) subgroups of the nearest OB association: Scorpius-Centaurus. The primary goals of the survey are to determine the star formation history of the OB subgroups and to assess the frequency of accreting stars in a sample dominated by "post–T Tauri" pre–main-sequence (PMS) stars. We investigate two samples: (1) proper-motion candidates from the ACT Catalog and Tycho Reference Catalog (TRC) with X-ray counterparts in the ROSAT All-Sky Survey (RASS) Bright Source Catalog and (2) G- and K-type stars in the Hipparcos catalog found to be candidate members by de Zeeuw et al. We obtained optical spectra of 130 candidates with the Siding Spring 2.3 m dual-beam spectrograph. PMS stars were identified by (1) strong Li λ6707 absorption, (2) subgiant surface gravities, (3) proper motions consistent with Sco-Cen membership, and (4) H-R diagram positions consistent with being PMS. We find 93% of the RASS-ACT/TRC stars to be probable PMS members, compared with 73% of the Hipparcos candidates. We demonstrate that measuring the gravity-sensitive band ratio of Sr II λ4077 to Fe I λ4071 is a valuable means of discriminating PMS and zero-age main-sequence (ZAMS) stars. Using secular parallaxes and Hipparcos , Tycho-2, and Two Micron All Sky Survey photometry, we construct an H-R diagram. Depending on the choice of published evolutionary tracks, we find the mean ages of the PMS populations to range between 17 and 23 Myr for LCC and 15 and 22 Myr for UCL. Taking into account observational errors, it appears that 95% of the low-mass star formation in each subgroup must have occurred in less than 8 Myr (LCC) and 12 Myr (UCL). Using the Bertelli et al. tracks, we find main-sequence turnoff ages for Hipparcos B-type members to be 16 ± 1 Myr for LCC and 17 ± 1 Myr for UCL. Contrary to previous findings, it appears that LCC is coeval with, or slightly older than, UCL. The secular parallaxes of the Sco-Cen PMS stars yield distances of 85–215 pc, with 12 of the LCC members lying within 100 pc of the Sun. Only one out of 110 (0.9 %; 1 σ) PMS solar-type stars in the sample with ages of 13 ± 1 (s.e.) ± 6 (1 σ) Myr and masses of 1.3 ± 0.2 (1 σ) M ⊙ shows both enhanced Hα emission and a K -band excess indicative of accretion from a truncated circumstellar disk: the nearby ( d ≃ 86 pc) classical T Tauri star PDS 66.
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A K5-type star with rotation period 3.20 days would be predicted to have soft X-ray emission around the saturation level (log(L_X/L_bol) = -3.2 +/- 0.3), perfectly consistent with the observed ROSAT X-ray flux (log(L_X/L_bol) = -3.2), and consistent with other Sco-Cen pre-MS stars.
“A K5-type star with rotation period of 3.20 days would be predicted to have soft X-ray emission around the saturation level (log(L X /L bol ) -3.2 ± 0.3; Pizzolato et al. 2003), perfectly consistent with the observed ROSAT X-ray flux (log(L X /L bol ) -3.2), and consistent with other Sco-Cen pre-MS stars (Mamajek et al. 2002).”
From PLANETARY CONSTRUCTION ZONES IN OCCULTATION: DISCOVERY OF AN EXTRASOLAR RING SYSTEM TRANSITING A YOUNG SUN-LIKE STAR AND FUTURE PROSPECTS FOR DETECTING ECLIPSES BY CIRCUMSECONDARY AND CIRCUMPLANETARY DISKS (2012) · cites this paper as Mamajek et al. 2002
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A Moving Cluster Distance to the Exoplanet 2M1207b in the TW Hydrae Association
Mamajek, E. E. (2005) · The Astrophysical Journal · doi:10.1086/468181 · Cited by 232 · see citing works
“There have been suggestions that some TWA stars may actually be background members of the ∼16-Myr-old Lower Centaurus-Crux (LCC) OB subgroup at d ≃ 110 pc (e.g. Mamajek & Feigelson 2001; Mamajek et al. 2002).”
BackgroundSelf-citationGiant planet companion to 2MASSW J1207334-393254
Chauvin, G., Lagrange, A. ‐., Dumas, C., Zuckerman, B., Mouillet, D., Song, I., Beuzit, J.-L., & Lowrance, P. (2005) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361:200500116/pdf · Cited by 234 · see citing works
A CHARA ARRAY SURVEY OF CIRCUMSTELLAR DISKS AROUND NEARBY Be-TYPE STARS
Touhami, Y. N., Gies, D. R., Schaefer, G. H., McAlister, H. A., Ridgway, S. T., Richardson, N. D., Matson, R. A., Grundstrom, E. D., ten Brummelaar, T. A., Goldfinger, P. J., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/768/2/128 · Cited by 228 · see citing works
Nearby Debris Disk Systems with High Fractional Luminosity Reconsidered
Moor, A., Abraham, P., Derekas, A., Kiss, C., Kiss, L. L., Apai, D., Grady, C., & Henning, T. K. (2006) · The Astrophysical Journal · doi:10.1086/503381 · Cited by 224 · see citing works
Metchev, S., & Hillenbrand, L. A. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/181/1/62 · Cited by 223 · see citing works
NEW DEBRIS DISKS AROUND YOUNG, LOW-MASS STARS DISCOVERED WITH THESPITZER SPACE TELESCOPE
Plavchan, P., Werner, M. W., Chen, C. H., Stapelfeldt, K. R., Su, K. Y. L., Stauffer, J. R., & Song, I. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/698/2/1068 · Cited by 209 · see citing works
Cieza, L. A., Padgett, D. L., Stapelfeldt, K. R., Augereau, J. ‐., Harvey, P. M., Evans, N. J., Merín, B., Koerner, D. W., Sargent, A. I., van Dishoeck, E. F., et al. (2007) · The Astrophysical Journal · doi:10.1086/520698 · Cited by 206 · see citing works
Bouwman, J., Henning, T. K., Hillenbrand, L. A., Meyer, M. R., Pascucci, I., Carpenter, J. M., Hines, D. C., Kim, J. S., Silverstone, M. D., Hollenbach, D. J., et al. (2008) · The Astrophysical Journal · doi:10.1086/587793 · Cited by 200 · see citing works
Self-citationMohanty, S., Jayawardhana, R., & Basri, G. S. (2005) · CERN Document Server (European Organization for Nuclear Research) · Cited by 196 · see citing works
THE COUPLED PHYSICAL STRUCTURE OF GAS AND DUST IN THE IM Lup PROTOPLANETARY DISK
Cleeves, L. I., Öberg, K. I., Wilner, D. J., Huang, J., Loomis, R. A., Andrews, S. M., & Czekala, I. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/832/2/110 · Cited by 177 · see citing works
The primordial binary population
Kouwenhoven, M. B. N., Brown, A. G. A., Zinnecker, H., Kaper, L., & Zwart, S. P. (2005) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20048124 · Cited by 186 · see citing works
XO-2b: Transiting Hot Jupiter in a Metal-rich Common Proper Motion Binary
Burke, C. J., McCullough, P. R., Valenti, J., Johns-Krull, C., Janes, K. A., Heasley, J., Summers, F. J., Stys, J., Bissinger, R., Fleenor, M., et al. (2007) · The Astrophysical Journal · doi:10.1086/523087 · Cited by 11,857 · see citing works
Asteroseismology for “à la carte” stellar age-dating and weighing
Lebreton, Y., & Goupil, M. J. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201423797 · Cited by 173 · see citing works
An, D., Terndrup, D. M., Pinsonneault, M. H., Paulson, D. B., Hanson, R. B., & Stauffer, J. R. (2007) · The Astrophysical Journal · doi:10.1086/509653 · Cited by 165 · see citing works
Astrophysics of Young Star Binaries
Prato, L. A., Greene, T. P., & Simon, M. (2003) · The Astrophysical Journal · doi:10.1086/345828 · Cited by 165 · see citing works
High-Dispersion Optical Spectra of Nearby Stars Younger Than the Sun
White, R. J., Gabor, J. M., & Hillenbrand, L. A. (2007) · The Astronomical Journal · doi:10.1086/514336 · Cited by 161 · see citing works
THE COLLISIONAL EVOLUTION OF DEBRIS DISKS
Gáspár, A., Rieke, G., & Balog, Z. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/768/1/25 · Cited by 98 · see citing works
The CIDA Variability Survey of Orion OB1. I. The Low-Mass Population of Ori OB1a and 1b
Briceño, C. A., Calvet, N., Hernández, J., Vivas, A. K., Hartmann, L. W., Downes, J. J., & Berlind, P. (2005) · The Astronomical Journal · doi:10.1086/426911 · Cited by 144 · see citing works
The kinematics of the Scorpius-Centaurus OB association from Gaia DR1
Wright, N. J., & Mamajek, E. E. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty207 · Cited by 144 · see citing works
Self-citationNearby debris disk systems with high fractional luminosity reconsidered
Moór, A., Ábrahám, P., Apai, D., Derekas, A., Grady, C., Henning, T. K., Kiss, C., & Kiss, L. L. (2006) · CERN Document Server (European Organization for Nuclear Research) · Cited by 144 · see citing works
Mamajek, E. E., Quillen, A. C., Pecaut, M. J., Moolekamp, F., Scott, E. L., Kenworthy, M. A., Cameron, A. C., & Parley, N. R. (2012) · The Astronomical Journal · doi:10.1088/0004-6256/143/3/72 · Cited by 140 · see citing works
“Factoring in previous age estimates for the UCL subgroup (see summary in Mamajek et al. 2002), and new age estimates using the F-star MS turnon (Pecaut, Mamajek, & Bubar 2011), we estimate the mean age of UCL to be 16 Myr with a ±2 Myr (68%CL) systematic uncertainty.”
MethodResultInfluentialSelf-citationChen, C. H., Mamajek, E. E., Bitner, M. A., Pecaut, M., Su, K. Y. L., & Weinberger, A. J. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/738/2/122 · Cited by 138 · see citing works
Self-citationNear-infrared cross-dispersed spectroscopy of brown dwarf candidates in the Upper Sco association★
Lodieu, N., Hambly, N. C., Jameson, R. F., & Hodgkin, S. T. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.12676.x · Cited by 139 · see citing works
Pascucci, I., Gorti, U., Hollenbach, D. J., Najita, J., Meyer, M. R., Carpenter, J. M., Hillenbrand, L. A., Herczeg, G. J., Padgett, D. L., Mamajek, E. E., et al. (2006) · The Astrophysical Journal · doi:10.1086/507761 · Cited by 132 · see citing works
Self-citationDetection of [Ne ii ] Emission from Young Circumstellar Disks
Pascucci, I., Hollenbach, D. J., Najita, J., Muzerolle, J. C., Gorti, U., Herczeg, G. J., Hillenbrand, L. A., Kim, J. S., Carpenter, J. M., Meyer, M. R., et al. (2007) · The Astrophysical Journal · doi:10.1086/518535 · Cited by 135 · see citing works
Self-citationSEARCHING FOR YOUNG M DWARFS WITHGALEX
Shkolnik, E. L., Liu, M. C., Reid, I. N., Dupuy, T. J., & Weinberger, A. J. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/727/1/6 · Cited by 134 · see citing works
Sartori, M. J., Lépine, J. R. D., & Dias, W. S. (2003) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20030581 · Cited by 133 · see citing works
Kouwenhoven, M. B. N., Brown, A. G. A., Zwart, S. P., & Kaper, L. (2007) · UvA-DARE (University of Amsterdam) · doi:10.1051/0004-6361:20077719 · Cited by 130 · see citing works
Silverstone, M. D., Meyer, M. R., Mamajek, E. E., Hines, D. C., Hillenbrand, L. A., Najita, J., Pascucci, I., Bouwman, J., Kim, J. S., Carpenter, J. M., et al. (2006) · The Astrophysical Journal · doi:10.1086/499418 · Cited by 126 · see citing works
Self-citationSHORT DISSIPATION TIMES OF PROTO-PLANETARY DISKS: AN ARTIFACT OF SELECTION EFFECTS?
Pfalzner, S., Steinhausen, M., & Menten, K. (2014) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/793/2/l34 · Cited by 120 · see citing works
A FAR-ULTRAVIOLET ATLAS OF LOW-RESOLUTIONHUBBLE SPACE TELESCOPESPECTRA OF T TAURI STARS
Yang, H., Herczeg, G. J., Linsky, J. L., Brown, A., Johns-Krull, C. M., Ingleby, L., Calvet, N., Bergin, E. A., & Valenti, J. A. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/744/2/121 · Cited by 121 · see citing works
On the distance to the Ophiuchus star‐forming region
Mamajek, E. E. (2008) · Astronomische Nachrichten · doi:10.1002/asna.200710827 · Cited by 118 · see citing works
Self-citationAccretion Rates for T Tauri Stars Using Nearly Simultaneous Ultraviolet and Optical SpectraPreprint
Ingleby, L. D., Calvet, N., Herczeg, G. J., Blaty, A., Walter, F. M., Ardila, D. R., Alexander, R. D., Edwards, S., Espaillat, C. C., Gregory, S. G., et al. (2013) · Cited by 116 · see citing works
Kerr, R. M. P., Rizzuto, A. C., Kraus, A. L., & Offner, S. S. R. (2021) · The Astrophysical Journal · doi:10.3847/1538-4357/ac0251 · Cited by 112 · see citing works
Evolution of Cold Circumstellar Dust around Solar-type Stars
Carpenter, J., Wolf, S., Schreyer, K., Launhardt, R., & Henning, T. (2004) · The Astronomical Journal · doi:10.1086/427131 · Cited by 93 · see citing works
Rizzuto, A. C., Newton, E. R., Mann, A. W., Tofflemire, B. M., Vanderburg, A. M., Kraus, A. L., Wood, M. L., Quinn, S. N., Zhou, G., Thao, P. C., et al. (2020) · The Astronomical Journal · doi:10.3847/1538-3881/ab94b7 · Cited by 110 · see citing works
Kraus, A. L., & Hillenbrand, L. A. (2007) · The Astrophysical Journal · doi:10.1086/516835 · Cited by 110 · see citing works
The Origin of the β Pictoris Moving Group
Ortega, V. G., Reza, R. D. L., Jilinski, E. G., & Bazzanella, B. (2002) · The Astrophysical Journal · doi:10.1086/342742 · Cited by 109 · see citing works
Mamajek, E. E., Meyer, M. R., Hinz, P. M., Hoffmann, W. F., Cohen, M., & Hora, J. L. (2004) · The Astrophysical Journal · doi:10.1086/422550 · Cited by 105 · see citing works
Self-citationMeyer, M. R., Carpenter, J. M., Mamajek, E. E., Hillenbrand, L. A., Hollenbach, D. J., Moro‐Martín, A., Kim, J. S., Silverstone, M. D., Najita, J., Hines, D. C., et al. (2008) · The Astrophysical Journal · doi:10.1086/527470 · Cited by 105 · see citing works
Self-citationASpitzerStudy of Dusty Disks in the Scorpius‐Centaurus OB Association
Chen, C., Jura, M. A., Gordon, K. D., & Blaylock, M. (2005) · The Astrophysical Journal · doi:10.1086/428607 · Cited by 103 · see citing works
On the kinematic evolution of young local associations and the Scorpius-Centaurus complex
Fernández, D., Figueras, F., & Torra, J. (2008) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20077720 · Cited by 102 · see citing works
X-ray emission from MP Muscae: an old classical T Tauri star
Argiroffi, C., Maggio, A., & Peres, G. (2007) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20067016 · Cited by 102 · see citing works
Desidera, S., Covino, E., Messina, S., Carson, J., Hagelberg, J., Schlieder, J., Biazzo, K., Alcalá, J., Chauvin, G., Vigan, A., et al. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201323168 · Cited by 70 · see citing works
Self-citationRe-examining the membership and origin of the ϵ Cha association
Murphy, S. J., Lawson, W. A., & Bessell, M. S. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1375 · Cited by 99 · see citing works
The Formation and Evolution of Planetary Systems: Placing Our Solar System in Context withSpitzer
Meyer, M. R., Hillenbrand, L. A., Backman, D., Beckwith, S., Bouwman, J., Brooke, T., Carpenter, J., Cohen, M., Cortes, S., Crockett, N., et al. (2006) · Publications of the Astronomical Society of the Pacific · doi:10.1086/510099 · Cited by 99 · see citing works
Self-citationHOT GAS LINES IN T TAURI STARS
Ardila, D. R., Herczeg, G. J., Gregory, S. G., Ingleby, L., France, K., Brown, A., Edwards, S., Johns-Krull, C., Linsky, J. L., Yang, H., et al. (2013) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/207/1/1 · Cited by 98 · see citing works
Stellar population of Sco OB2 revealed by <i>Gaia</i> DR2 data
Damiani, F., Prisinzano, L., Pillitteri, I., Micela, G., & Sciortino, S. (2019) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201833994 · Cited by 97 · see citing works
OB Associations and their origins
Wright, N. J. (2020) · New Astronomy Reviews · doi:10.1016/j.newar.2020.101549 · Cited by 96 · see citing works
The ε Chamaeleontis Young Stellar Group and the Characterization of Sparse Stellar Clusters
Feigelson, E. D., Lawson, W. A., & GARMIRE, G. P. (2003) · The Astrophysical Journal · doi:10.1086/379365 · Cited by 95 · see citing works
Circumstellar Dust Created by Terrestrial Planet Formation in HD 113766
Lisse, C. M., Chen, C. H., Wyatt, M. C., & Morlok, A. (2008) · The Astrophysical Journal · doi:10.1086/523626 · Cited by 94 · see citing works
DISTANCE AND KINEMATICS OF THE TW HYDRAE ASSOCIATION FROM PARALLAXES
Weinberger, A. J., Anglada-Escudé, G., & Boss, A. P. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/762/2/118 · Cited by 93 · see citing works
X-shooter survey of disk accretion in Upper Scorpius
Manara, C. F., Natta, A., Rosotti, G. P., Alcalá, J. M., Nisini, B., Lodato, G., Testi, L., Pascucci, I., Hillenbrand, L. A., Carpenter, J. M., et al. (2020) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202037949 · Cited by 93 · see citing works
PROBING STELLAR ACCRETION WITH MID-INFRARED HYDROGEN LINES
Rigliaco, E., Pascucci, I., Duchêne, G., Edwards, S., Ardila, D. R., Grady, C., Mendigutía, I., Montesinos, B., Mulders, G. D., Najita, J. R., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/801/1/31 · Cited by 92 · see citing works
Self-citationPatel, R. I., Metchev, S., & Heinze, A. (2014) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/212/1/10 · Cited by 90 · see citing works
Hot Jupiters and the evolution of stellar angular momentum
Lanza, A. F. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200912789 · Cited by 90 · see citing works
Revised Filter Profiles and Zero Points for Broadband Photometry
Mann, A. W., & von Braun, K. (2015) · Publications of the Astronomical Society of the Pacific · doi:10.1086/680012 · Cited by 89 · see citing works
On the kinematic evolution of young local associations and the Scorpius-Centaurus complex
Fernández, D., Figueras, F., & Torra, J. (2008) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361:20077720/pdf · Cited by 89 · see citing works
WIDE COOL AND ULTRACOOL COMPANIONS TO NEARBY STARS FROM Pan-STARRS 1
Deacon, N. R., Liu, M. C., Magnier, E. A., Aller, K. M., Best, W. M. J., Dupuy, T., Bowler, B. P., Mann, A. W., Redstone, J. A., Burgett, W. S., et al. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/792/2/119 · Cited by 88 · see citing works
Matrà, L., Panić, O., Wyatt, M. C., & Dent, W. R. F. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu2619 · Cited by 87 · see citing works
Further identification of ROSAT all-sky survey sources in Orion
Frasca, A., Alcalá, J. M., Covino, E., Catalano, S., Marilli, E., & Paladino, R. (2003) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20030644 · Cited by 87 · see citing works
Rizzuto, A. C., Newton, E. R., Mann, A. W., Tofflemire, B. M., Vanderburg, A. M., Kraus, A. L., Wood, M. L., Quinn, S. N., Zhou, G., Thao, P. C., et al. (2020) · Cited by 86 · see citing works
Detection of a transit by the planetary companion of HD 80606
Fossey, S. J., Waldmann, I. P., & Kipping, D. (2009) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1111/j.1745-3933.2009.00653.x · Cited by 85 · see citing works
Hot Jupiters and the evolution of stellar angular momentumPreprint
Lanza, A. F. (2009) · Cited by 85 · see citing works
SPECTROSCOPIC CHARACTERIZATION OF HD 95086 b WITH THE GEMINI PLANET IMAGER
Rosa, R. J. D., Rameau, J., Patience, J., Graham, J. R., Doyon, R., Lafreniére, D., Macintosh, B., Pueyo, L. A., Rajan, A., Wang, J., et al. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/824/2/121 · Cited by 73 · see citing works
The X-ray soft excess in classical T Tauri stars
Güdel, M., & Telleschi, A. (2007) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20078143 · Cited by 81 · see citing works
The Formation and Evolution of Planetary Systems: Description of theSpitzerLegacy Science Database
Carpenter, J. M., Bouwman, J., Silverstone, M. D., Kim, J. S., Stauffer, J. R., Cohen, M., Hines, D. C., Meyer, M. R., & Crockett, N. R. (2008) · The Astrophysical Journal Supplement Series · doi:10.1086/592274 · Cited by 81 · see citing works
Self-citationMittal, T., Chen, C., Jang‐Condell, H., Manoj, P., Sargent, B. A., Watson, D. M., & Lisse, C. M. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/798/2/87 · Cited by 78 · see citing works
Gagné, J., Faherty, J. K., Mamajek, E. E., Malo, L., Doyon, R., Filippazzo, J., Weinberger, A. J., Donaldson, J. K., Lépine, S., Lafreniére, D., et al. (2017) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/228/2/18 · Cited by 80 · see citing works
Self-citationEvolution of Cold Circumstellar Dust Around Solar-Type Stars
Carpenter, J. M., Wolf, S., Schreyer, K., Launhardt, R., & Henning, T. K. (2004) · CERN Document Server (European Organization for Nuclear Research) · Cited by 77 · see citing works
Lebreton, Y., & Goupil, M.-J. (2014) · arXiv (Cornell University) · doi:10.48550/arxiv.1406.0652 · Cited by 75 · see citing works
Multiwavelength diagnostics of accretion in an X-ray selected sample of CTTSs
Curran, R., Argiroffi, C., Sacco, G. G., Orlando, S., Peres, G., Reale, F., & Maggio, A. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201015522 · Cited by 74 · see citing works
The Evolution of Disk Winds from a Combined Study of Optical and Infrared Forbidden Lines
Pascucci, I., Banzatti, A., Gorti, U., Fang, M., Pontoppidan, K. M., Alexander, R. D., Ballabio, G., Edwards, S., Salyk, C., Sacco, G. G., et al. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/abba3c · Cited by 72 · see citing works
Self-citationA Census of the Stellar Populations in the Sco-Cen Complex*
Luhman, K. L. (2021) · The Astronomical Journal · doi:10.3847/1538-3881/ac35e2 · Cited by 72 · see citing works
Rotational velocities of nearby young stars
Weise, P., Launhardt, R., Setiawan, J., & Henning, T. K. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201014453 · Cited by 72 · see citing works
Revised filter profiles and zero points for broadband photometry
Mann, A. W., & von Braun, K. (2015) · Max Planck Institute for Plasma Physics · Cited by 72 · see citing works
BANYAN. XII. New Members of Nearby Young Associations from GAIA–Tycho Data
Gagné, J., Roy-Loubier, O., Faherty, J. K., Doyon, R., & Malo, L. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aac2b8 · Cited by 71 · see citing works
Distance and Kinematics of the TW Hydrae Association from ParallaxesPreprint
Weinberger, A. J., & Boss, A. P. (2016) · Cited by 69 · see citing works
Kuiper belts around nearby stars
Nilsson, R., Liseau, R., Brandeker, A., Olofsson, G., Pilbratt, G. L., Risacher, C., Rodmann, J., Augereau, J. ‐., Bergman, P., Eiroa, C., et al. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201014444 · Cited by 68 · see citing works
Slingshot prominences: nature’s wind gauges
Jardine, M., & Cameron, A. C. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty2872 · Cited by 68 · see citing works
A seismic and gravitationally bound double star observed byKepler
Appourchaux, T. P., Antia, H. M., Ball, W. H., Creevey, O. L., Lebreton, Y., Verma, K., Vorontsov, S. V., Campante, T. L., Davies, G. R., Gaulme, P., et al. (2015) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201526610 · Cited by 67 · see citing works
The widest Hα survey of accreting protoplanets around nearby transition disks
Zurlo, A., Cugno, G., Montesinos, M., Perez, S., Cánovas, H., Casassus, S., Christiaens, V., Cieza, L., & Huelamo, N. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201936891 · Cited by 69 · see citing works
Photometric study of the young open cluster NGC 3293
Baume, G., Vázquez, R. A., B, G. C. A., & Feinstein, A. (2003) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20030223 · Cited by 66 · see citing works
51 Eridani and GJ 3305: A 10-15 Myr old Binary Star System at 30 Parsecs
Feigelson, E. D., Lawson, W. A., Stark, M., Townsley, L., & GARMIRE, G. P. (2006) · The Astronomical Journal · doi:10.1086/499923 · Cited by 64 · see citing works
- Authors
- Mamajek, E. E., Meyer, M. R., & Liebert, J.
- Affiliations
- University of Arizona (US)
- Venue
- The Astronomical Journal
- Publisher
- American Astronomical Society
- Published
- 2002-09
- Volume
- 124
- Issue
- 3
- Pages
- 1670-1694
- ISSN
- 0004-6256 (ISSN-L)
- 1538-3881
- OpenAlex
- W2016878712
- Semantic Scholar
- 30fce1ce0f1048bc39ba98a01037605839457dc0
- Cited by
- 310
- References
- 74
- Citations by year
- 2026: 5 · 2025: 12 · 2024: 10 · 2023: 9 · 2022: 5 · 2021: 13 · 2020: 20 · 2019: 11 · 2018: 15 · 2017: 10 · 2016: 15 · 2015: 12 · 2014: 17 · 2013: 17 · 2012: 11
- FWCI
- 8.02
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- The Astronomical Journal (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Funders
- National Science Foundation
- National Aeronautics and Space Administration
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
- Keywords
- post-T Tauri stars, pre-main-sequence stars, Scorpius-Centaurus OB association, star formation history, accretion, lithium absorption, stellar ages, X-ray sources, low-mass star formation
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
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Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
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