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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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Cited by
Sorted by citations
MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS
Choi, J., Dotter, A., Conroy, C., Cantiello, M., Paxton, B., & Johnson, B. D. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/823/2/102 · Cited by 2,922
Gagné, J., Mamajek, E. E., Malo, L., Riedel, A. R., Rodriguez, D., Lafreniére, D., Faherty, J. K., Roy-Loubier, O., Pueyo, L. A., Robin, A. C., et al. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aaae09 · Cited by 565
Self-citationPecaut, M. J., Mamajek, E. E., & Bubar, E. J. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/746/2/154 · Cited by 564
“UCL Interlopers Chen et al. (2011) reject HIP 70833 as a member of UCL since the cooler K3IV companion has an EW(Li λ6707Å) of only 0.01 Å.”
BackgroundMethodInfluentialSelf-citationPecaut, M. J., & Mamajek, E. E. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1300 · Cited by 407
Self-citationBAYESIAN ANALYSIS TO IDENTIFY NEW STAR CANDIDATES IN NEARBY YOUNG STELLAR KINEMATIC GROUPS
Malo, L., Doyon, R., Lafreniére, D., Artigau, É., Gagné, J., Baron, F., & Riedel, A. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/762/2/88 · Cited by 361
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
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.
Statistics and arithmetic are recomputed, not judged.
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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