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Related papers: Debris Disk Evolution Around A Stars

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We present a study of the evolution of the inner few astronomical units of protoplanetary disks around low-mass stars. We consider nearby stellar groups with ages spanning from 1 to 11 Myr, distributed into four age bins. Combining…

We observed 69 A3-F8 main sequence binary star systems using the Multiband Imaging Photometer for Spitzer onboard the Spitzer Space Telescope. We find emission significantly in excess of predicted photospheric flux levels for 9(+4/-3)% and…

We have conducted a study of debris disks around F stars in order to explore correlations between rotation, stellar winds, and circumstellar disks. We obtained new 24 micron photometry from Spitzer's Multiband Imaging Photometer for Spitzer…

Solar and Stellar Astrophysics · Physics 2015-06-11 Trisha Mizusawa , Luisa Rebull , John Stauffer , Geoffrey Bryden , Michael Meyer , Inseok Song

We use Spitzer Space Telescope 24 {\mu}m data to search for debris disks among 122 AFGKM stars from the \sim 670 Myr clusters Hyades, Coma Ber, and Praesepe, utilizing a number of advances in data reduction and determining the intrinsic…

Astrophysics of Galaxies · Physics 2012-04-24 Laurie Urban , George Rieke , Kate Su , David E. Trilling

As part of a large Spitzer/MIPS GTO program, we have searched for infrared excesses due to debris disks toward 26 FGK field stars known from radial velocity (RV) studies to have one or more planets. While none of these stars show excesses…

Debris disks with extremely large infrared excesses (fractional luminosities $> 10^{-2}$) are rare. Those with ages between 30 and 130 Myr are of interest because their evolution has progressed well beyond that of protoplanetary disks…

Earth and Planetary Astrophysics · Physics 2012-05-07 Huan Y. A. Meng , George H. Rieke , Kate Y. L. Su , Valentin D. Ivanov , Leonardo Vanzi , Wiphu Rujopakarn

(abbreviated) We report detection with the Spitzer Space Telescope of cool dust surrounding solar type stars. The observations were performed as part of the Legacy Science Program, ``Formation and Evolution of Planetary Systems'' (FEPS).…

We present 24 micron photometry of the intermediate-age open cluster Praesepe. We assemble a catalog of 193 probable cluster members that are detected in optical databases, the Two Micron All Sky Survey (2MASS), and at 24 micron, within an…

Solar and Stellar Astrophysics · Physics 2010-01-15 A. Gaspar , G. H. Rieke , K. Y. L. Su , Z. Balog , D. Trilling , J. Muzzerole , D. Apai , B. C. Kelly

We present Multiband Imaging Photometer for Spitzer (MIPS) observations at 24 and 70 microns for 30 stars, and at 160 microns for a subset of 12 stars, in the nearby (~30 pc), young (~12 Myr) Beta Pictoris Moving Group (BPMG). In several…

Context. Little is known about the properties of the warm (Tdust >~ 150 K) debris disk material located close to the central star, which has a more direct link to the formation of terrestrial planets than the low temperature debris dust…

We report Spitzer Space Telescope IRAC 3.6, 4.5, 5.8 and 8 um and MIPS 24 and 70 um observations of the 32 Ori Group, a recently discovered nearby stellar association situated towards northern Orion. The proximity of the group (~93 pc) has…

Solar and Stellar Astrophysics · Physics 2016-12-22 Alexander J. Shvonski , Eric E. Mamajek , Jinyoung Serena Kim , Michael R. Meyer , Mark J. Pecaut

We present the optical to mid-infrared SEDs of 11 debris disk candidates from $Spitzer$ SWIRE fields. All these candidates are selected from SWIRE 24$\mu$m sources matched with both the SDSS star catalog and the 2MASS point source catalog.…

Solar and Stellar Astrophysics · Physics 2015-06-04 Hong Wu , Chao-Jian Wu , Chen Cao , Sebastian Wolf , Jing-Yao Hu

We present 4.5, 8, and 16um photometry from the Spitzer Space Telescope for 204 stars in the Upper Scorpius OB Association. The data are used to investigate the frequency and properties of circumstellar disks around stars with masses…

Astrophysics · Physics 2011-02-11 John M. Carpenter , Eric E. Mamajek , Lynne A. Hillenbrand , Michael R. Meyer

Motivated by the reported dearth of debris discs around M stars, we use survival models to study the occurrence of planetesimal discs around them. These survival models describe a planetesimal disc with a small number of parameters,…

Earth and Planetary Astrophysics · Physics 2015-06-15 Kevin Heng , Matej Malik

(Abridged) Studies of debris discs have shown that most systems are analogous to the EKB. In this study we aim to determine how many IRAS 25um excesses towards A stars are real, and investigate where the dust lies. We observe with TIMMI2,…

Earth and Planetary Astrophysics · Physics 2015-05-18 R. Smith , M. C. Wyatt

Spitzer Space Observatory IRAC and MIPS photometric observations are presented for 20 white dwarfs with T < 20,000 K and metal-contaminated photospheres. A warm circumstellar disk is detected at GD 16 and likely at PG 1457-086, while the…

Earth and Planetary Astrophysics · Physics 2011-02-11 J. Farihi , M. Jura , B. Zuckerman

We have bandmerged candidate transiting planetary systems (from the Kepler satellite) and confirmed transiting planetary systems (from the literature) with the recent Wide-field Infrared Survey Explorer (WISE) preliminary release catalog.…

Earth and Planetary Astrophysics · Physics 2013-12-03 Álvaro Ribas , Bruno Merín , David R. Ardila , Hervé Bouy

We present the discovery of debris systems around three solar mass stars based upon observations performed with the Spitzer Space Telescope as part of a Legacy Science Program, ``the Formation and Evolution of Planetary Systems'' (FEPS). We…

Using ISO-ISOPHOT we carried out a survey of almost 150 stars to search for evidence of emission from dust orbiting young main sequence stars, both in clusters and isolated systems. Over half of the detections are new examples of dusty…

Astrophysics · Physics 2010-03-19 C. Spangler , A. I. Sargent , M. D. Silverstone , E. E. Becklin , B. Zuckerman

We present the results of a survey of young intermediate mass stars (age $<$~5 Myr, 1.5 $<M_{\star} \leq $ 15 $M_{\odot}$) in the W5 massive star forming region. We use combined optical, near-infrared and {\it Spitzer} Space Telescope…

Astrophysics of Galaxies · Physics 2015-05-20 Xavier P. Koenig , Lori E. Allen