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A MAGELLAN MIKE AND SPITZER MIPS STUDY OF 1.5-1.0 M☉STARS IN SCORPIUS-CENTAURUS
Open accessAbstract
We obtained Spitzer Space Telescope Multiband Imaging Photometer for Spitzer (MIPS) 24 μm and 70 μm observations of 182 nearby, Hipparcos F-and G-type common proper motion single and binary systems in the nearest OB association, Scorpius-Centaurus.We also obtained Magellan/MIKE R ∼ 50,000 visual spectra at 3500-10500 Å for 181 candidate ScoCen stars in single and binary systems.Combining our MIPS observations with those of other ScoCen stars in the literature, we estimate 24 μm F+G-type disk fractions of 9/27 (33% ± 11%), 21/67 (31% ± 7%), and 25/71 (35% ± 7%) for Upper Scorpius (∼10 Myr), Upper Centaurus Lupus (∼15 Myr), and Lower Centaurus Crux (∼17 Myr), respectively.We confirm previous IRAS and MIPS excess detections and present new discoveries of 41 protoplanetary and debris disk systems, with fractional infrared luminosities ranging from L IR /L * = 10 -5 to 10 -2 and grain temperatures ranging from T gr = 40-300 K.We searched for an increase in 24 μm excess at an age of 15-20 Myr, consistent with the onset of debris production predicted by coagulation N-body simulations of outer planetary systems.We found such an increase around 1.5 M stars but discovered a decrease in the 24 μm excess around 1.0 M stars.We additionally discovered that the 24 μm excess around 1.0 M stars is larger than predicted by self-stirred models.Finally, we found a weak anti-correlation between fractional infrared luminosity (L IR /L * ) and chromospheric activity (R HK ), that may be the result of differences in stellar properties, such as mass, luminosity, and/or winds.
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“Using the Upper Cen-Lup (UCL) subgroup velocity vector from Chen et al. (2011) ( U, V, W = -5.1 ± 0.6, -19.7 ± 0.4, -4.6 ± 0.3 km s -1 ), we predict the RV of an ideal UCL member at the position of J1407 to be γ = 7.0 km s -1 , with a predicted rms scatter amongst members of ± 1.3 kms -1 .”
From Mass and period limits on the ringed companion transiting the young star J1407 (2015) · cites this paper as Chen et al. 2011
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Jang‐Condell, H., Chen, C., Mittal, T., Manoj, P., Watson, D. M., Lisse, C. M., Nesvold, E., & Kuchner, M. J. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/808/2/167 · Cited by 37
Self-citationDesidera, S., Covino, E., Messina, S., Carson, J., Hagelberg, J., Schlieder, J. E., Biazzo, K., Alcalá, J. M., Chauvin, G., Vigan, A., et al. (2014) · arXiv (Cornell University) · doi:10.48550/arxiv.1405.1559 · Cited by 37
Mass and period limits on the ringed companion transiting the young star J1407
Kenworthy, M. A., Lacour, S., Kraus, A., Triaud, A. H. M. J., Mamajek, E. E., Scott, E. L., Ségransan, D., Ireland, M., Hambsch, F.-J., Reichart, D. E., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu2067 · Cited by 36
“Using the Upper Cen–Lup (UCL) subgroup velocity vector from Chen et al. (2011) (U, V,W = -5.1± 0.6, - 19.7± 0.4, -4.6± 0.3 km s−1), we predict the RV of an ideal UCL member at the position of J1407 to be γ = 7.0 km s−1, c© 2014 RAS, MNRAS 000, 1–20”
MethodInfluentialSelf-citationDavies, C. L. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz086 · Cited by 36
Kenyon, S. J., & Bromley, B. C. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/817/1/51 · Cited by 35
Nardiello, D. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa2745 · Cited by 37
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Self-citationHD 144548: A young triply eclipsing system in the Upper Scorpius OB association
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The First Scattered-light Image of the Debris Disk around the Sco–Cen Target HD 129590
Matthews, E. C., Hinkley, S., Vigan, A., Kennedy, G., Rizzuto, A. C., Stapelfeldt, K. R., Mawet, D. P., Booth, M., Chen, C., & Jang-Condell, H. (2017) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/aa7943 · Cited by 33
Self-citationThree-dimensional structure of the Upper Scorpius association with the Gaia first data release
Galli, P. A. B., Joncour, I., & Moraux, E. (2018) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/sly036 · Cited by 32
ROCKY PLANET FORMATION: QUICK AND NEAT
Kenyon, S. J., Najita, J. R., & Bromley, B. C. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/831/1/8 · Cited by 31
A DEEPSPITZERSURVEY OF CIRCUMSTELLAR DISKS IN THE YOUNG DOUBLE CLUSTER, h AND χ PERSEI
Cloutier, R., Currie, T., Rieke, G. H., Kenyon, S. J., Balog, Z., & Jayawardhana, R. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/796/2/127 · Cited by 29
A Near-coplanar Stellar Flyby of the Planet Host Star HD 106906
Rosa, R. J. D., & Kalas, P. (2019) · The Astronomical Journal · doi:10.3847/1538-3881/ab0109 · Cited by 30
Analysis of 1SWASP J140747.93−394542.6 eclipse fine-structure: hints of exomoons
van Werkhoven, T. I. M., Kenworthy, M. A., & Mamajek, E. E. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu725 · Cited by 29
Self-citationPre-main-sequence stars older than 8 Myr in the Eagle nebula
Marchi, G. D., Panagia, N., Guarcello, M. G., & Bonito, R. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1499 · Cited by 29
Detection of scattered light from the hot dust in HD 172555
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Spitzer’s debris disk legacy from main-sequence stars to white dwarfs
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Self-citationchronostar – II. Kinematic age and substructure of the Scorpius–Centaurus OB2 association
Žerjal, M., Ireland, M. J., Crundall, T. D., Krumholz, M. R., & Rains, A. D. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac3693 · Cited by 24
Lodieu, N., Alonso, R., Hernández, J. I. G., Sanchis-Ojeda, R., Narita, N., Kawashima, Y., Kawauchi, K., Mascareño, A. S., Deeg, H., Arranz, J. P., et al. (2015) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201527464 · Cited by 26
Copious Amounts of Hot and Cold Dust Orbiting the Main Sequence A-type Stars HD131488 and HD121191Preprint
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Su, K. Y. L., Rieke, G. H., Melis, C., Jackson, A. P., Smith, P. S., Meng, H., & Gáspár, A. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/ab9c9b · Cited by 25
Self-citationNew members of the TW Hydrae Association and two accreting M-dwarfs in Scorpius–Centaurus
Murphy, S. J., Lawson, W. A., & Bento, J. D. S. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1745 · Cited by 24
Gibbs, A., Wagner, K., Apai, D., Moór, A., Currie, T., Bonnefoy, M., Langlois, M., & Lisse, C. (2019) · The Astronomical Journal · doi:10.3847/1538-3881/aaf1bd · Cited by 24
A debris disc under the influence of a wide planetary-mass companion: the system of HD 106906
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Multiplicity of disc-bearing stars in Upper Scorpius and Upper Centaurus-Lupus
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Goebel, S. B., Currie, T., Guyon, O., Brandt, T. D., Groff, T. D., Jovanović, N., Kasdin, N. J., Lozi, J., Hodapp, K. W., Martinache, F., et al. (2018) · The Astronomical Journal · doi:10.3847/1538-3881/aaeb24 · Cited by 23
HD 144548: A young triply eclipsing system in the Upper Scorpius OB association
Alonso, R., Deeg, H. J., Hoyer, S., Lodieu, N., Πάλλη, Ε., & Sanchis-Ojeda, R. (2015) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201527109/pdf · Cited by 23
Searching for infrared excesses in Sun-like stars observed by WISE
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New binaries from the SHINE survey
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Detection of scattered light from the hot dust in HD 172555
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Evidence for Misalignment between Debris Disks and Their Host Stars
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THE NEARBY, YOUNG, ISOLATED, DUSTY STAR HD 166191
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Lodieu, N., Alonso, R., Hernández, J. I. G., Sanchis-Ojeda, R., Narita, N., Kawashima, Y., Kawauchi, K., Mascareño, A. S., Deeg, H. J., Prieto-Arranz, J., et al. (2015) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201527464/pdf · Cited by 19
Dynamical Masses of Young Stars. II. Young Taurus Binaries Hubble 4, FF Tau, and HP Tau/G3
Rizzuto, A. C., Dupuy, T. J., Ireland, M. J., & Kraus, A. L. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/ab5aed · Cited by 21
Metadata
- Authors
- Chen, C. H., Mamajek, E. E., Bitner, M. A., Pecaut, M., Su, K. Y. L., & Weinberger, A. J.
- Affiliations
- Space Telescope Science Institute (US)
- University of Rochester (US)
- University of Arizona (US)
- Carnegie Institution for Science (US)
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2011-08-18
- Volume
- 738
- Issue
- 2
- Pages
- 122
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2068806560
- Cited by
- 138
- References
- 86
- Citations by year
- 2026: 3 · 2025: 2 · 2023: 6 · 2022: 4 · 2021: 5 · 2020: 13 · 2019: 6 · 2018: 13 · 2017: 11 · 2016: 15 · 2015: 16 · 2014: 13 · 2013: 17 · 2012: 14
- FWCI
- 7.34
- Type
- journal article
- Language
- he
- Open access
- bronze
- doi.org
- Locations
- The Astrophysical Journal (publishedVersion)
- Funders
- National Aeronautics and Space Administration
- California Institute of Technology
- Jet Propulsion Laboratory
- 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
- Scorpius-Centaurus OB association, protoplanetary disks, debris disks, disk fraction, stellar ages, Upper Scorpius, Upper Centaurus Lupus, Lower Centaurus Crux, chromospheric activity, stellar winds, binary stars
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