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Related papers: Debris disks around Sun-like stars

200 papers

Stellar infrared excesses can indicate various phenomena of interest, from protoplanetary disks to debris disks, or (more speculatively) techno-signatures along the lines of Dyson spheres. In this paper, we conduct a large search for such…

Earth and Planetary Astrophysics · Physics 2024-09-20 Gabriella Contardo , David W. Hogg

The Spitzer Space Telescope has advanced debris disk science tremendously with a wealth of information on debris disks around nearby A, F, G, K and M stars at 24 and 70 microns with the MIPS photometer and at 8-34 microns with IRS. Here we…

Solar and Stellar Astrophysics · Physics 2015-05-13 Angelle Tanner , Charles Beichman , Geoff Bryden , Carey Lisse , Samantha Lawler

We have observed 152 nearby solar-type stars with the Infrared Spectrometer (IRS) on the Spitzer Space Telescope. Including stars that met our criteria but were observed in other surveys, we get an overall success rate for finding excesses…

Solar and Stellar Astrophysics · Physics 2014-11-20 S. M. Lawler , C. A. Beichman , G. Bryden , D. R. Ciardi , A. M. Tanner , K. Y. L. Su , K. R. Stapelfeldt , C. M. Lisse , D. E. Harker

Using data from the Spitzer Space Telescope Legacy Science Program ``Formation and Evolution of Planetary Systems'' (FEPS), we have searched for debris disks around 9 FGK stars (2-10 Gyr), known from radial velocity (RV) studies to have one…

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 cross-correlate \hip\ main-sequence star catalog with \fis\ catalog, and identify 136 stars (at $>90$% reliability) with far-infrared detections at least in one band. After rejecting 51 stars classified as young stellar objects, Be…

Earth and Planetary Astrophysics · Physics 2020-07-27 Qiong Liu , Tinggui Wang , Peng Jiang

We present MIPS 24um and 70um photometry for 205 members of the Upper Scorpius OB Association. These data are combined with published MIPS photometry for 15 additional association members to assess the frequency of circumstellar disks…

Solar and Stellar Astrophysics · Physics 2014-11-20 John M. Carpenter , Eric E. Mamajek , Lynne A. Hillenbrand , Michael R. Meyer

More than a thousand warm debris disks have been detected as infrared excess at mid-infrared wavelengths, and their frequencies have been obtained for various spectral types of stars. However, the dependence of the frequencies on spectral…

Earth and Planetary Astrophysics · Physics 2024-04-08 Toshiyuki Mizuki , Munetake Momose , Masataka Aizawa , Hiroshi Kobayashi

We present Spitzer photometric (IRAC and MIPS) and spectroscopic (IRS low resolution) observations for 314 stars in the Formation and Evolution of Planetary Systems (FEPS) Legacy program. These data are used to investigate the properties…

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 conducted a survey for infrared excess emission from 16 nearby main sequence shell stars using the Multiband Imaging Photometer for Spitzer (MIPS) on the Spitzer Space Telescope. Shell stars are early-type stars with narrow absorption…

Astrophysics · Physics 2010-11-11 Aki Roberge , Alycia J. Weinberger

We describe Spitzer IRAC and MIPS observations of the nearby 25 Myr-old open cluster NGC 2232. Combining these data with ROSAT All-Sky Survey observations, proper motions, and optical photometry/spectroscopy, we construct a list of highly…

Astrophysics · Physics 2009-11-13 Thayne Currie , Peter Plavchan , Scott J. Kenyon

We probe the effect of the ISM on debris disc occurrence rates and on the morphologies of the discs. We used results from the Herschel Space Observatory DUNES and DEBRIS surveys of 295 nearby FGK dwarf stars imaged at 100 $\mu$m and 160…

Earth and Planetary Astrophysics · Physics 2025-02-07 A. M. Heras , C. Eiroa , C. del Burgo , J. P. Marshall , B. Montesinos

We report the discovery of four rare debris disks with warm excesses around F-stars, significantly increasing the number of such systems known in the solar neighborhood. Three of the disks are consistent with the predictions of steady state…

Solar and Stellar Astrophysics · Physics 2009-08-05 A. Moór , D. Apai , I. Pascucci , P. Ábrahám , C. Grady , Th. Henning , A. Juhász , Cs. Kiss , Á. Kóspál

We present photometric ISO 60 and 170um measurements, complemented by some IRAS data at 60um, of a sample of 84 nearby main-sequence stars of spectral class A, F, G and K in order to determine the incidence of dust disks around such…

Circumstellar dust disks have been observed around many nearby stars. However, many stars are part of binary or multiple stellar systems. A natural question arises regarding the presence and properties of such disks in systems with more…

Solar and Stellar Astrophysics · Physics 2019-08-17 David R. Rodriguez , Gaspard Duchene , Henry Tom , Grant Kennedy , Brenda Matthews , Jane Greaves , Harold Butner

Context: Debris disks are important observational clues for understanding planetary-system formation process. In particular, faint warm debris disks may be related to late planet formation near 1 AU. A systematic search of faint warm debris…

We present an analysis of debris disk data around Solar-type stars (spectral types F0-K5) using the steady-state analytical model of Wyatt et al. (2007). Models are fitted to published data from the FEPS (Meyer et al. 2006) project and…

Solar and Stellar Astrophysics · Physics 2011-02-23 N. Kains , M. C. Wyatt , J. S. Greaves

We report the results of a spectroscopic search for debris disks surrounding 41 nearby solar type stars, including 8 planet-bearing stars, using the {\it Spitzer Space Telescope}. With accurate relative photometry using the Infrared…

We have surveyed the 30 Myr-old cluster NGC 2547 for planetary debris disks using Spitzer. At 4.5-8 um we are sensitive to the photospheric level down to mid-M stars (0.2 Msol) and at 24 um to early-G stars (1.2 Msol). We find only two to…

Astrophysics · Physics 2008-11-26 N. Gorlova , Z. Balog , G. H. Rieke , J. Muzerolle , K. Y. L. Su , V. D. Ivanov , E. T. Young