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相关论文: A Spitzer view of protoplanetary disks in the gamm…

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We present the results from an Atacama Large Millimeter/Submillimeter Array (ALMA) 1.3 mm continuum and $^{12}$CO ($J=2-1$) line survey spread over 10 square degrees in the Serpens star-forming region of 320 young stellar objects, 302 of…

太阳与恒星天体物理 · 物理学 2022-10-26 Alexa R. Anderson , Jonathan P. Williams , Nienke van der Marel , Charles J. Law , Luca Ricci , John J. Tobin , Simin Tong

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…

太阳与恒星天体物理 · 物理学 2015-05-13 Angelle Tanner , Charles Beichman , Geoff Bryden , Carey Lisse , Samantha Lawler

We have obtained Spitzer Space Telescope Multiband Imaging Photometer for Spitzer (MIPS) 24 {\mu}m and 70 {\mu}m observations of 215 nearby, Hipparcos B- and A-type common proper motion single and binary systems in the nearest OB…

太阳与恒星天体物理 · 物理学 2015-06-05 Christine H. Chen , Mark Pecaut , Eric E. Mamajek , Kate Y. L. Su , Martin Bitner

Recent high-resolution observations with the Hubble Space Telescope (HST) reveal that star clusters of extraordinary luminosity and compactness are commonly found in a variety of starburst systems. There has been much speculation that these…

天体物理学 · 物理学 2009-10-28 Luis C. Ho , Alexei V. Filippenko

(Abridged) Surveys of protoplanetary disks in nearby star-forming regions (SFRs) have provided important information on their demographics, but due to their sample sizes, they cannot be used to study how disk properties vary with the…

地球与行星天体物理 · 物理学 2022-05-11 S. E. van Terwisga , A. Hacar , E. F. van Dishoeck , R. Oonk , S. Portegies Zwart

We present ALMA observations of 106 G-, K-, and M-type stars in the Upper Scorpius OB Association hosting circumstellar disks. With these data, we measure the 0.88 mm continuum and $^{12}$CO $J$ = 3$-$2 line fluxes of disks around low-mass…

地球与行星天体物理 · 物理学 2016-08-31 Scott A. Barenfeld , John M. Carpenter , Luca Ricci , Andrea Isella

We present mid-infrared spectra between 5.2 and 38 microns for 26 disk-bearing members of the ~5 Myr old Upper Scorpius OB association obtained with the Infrared Spectrograph onboard the Spitzer Space Telescope. We find clear evidence for…

太阳与恒星天体物理 · 物理学 2009-11-13 S. E. Dahm , John M. Carpenter

(Abridged) We present results from a JCMT/SCUBA 850 um search for cold dust around nearby young stars belonging to the beta Pic (t~12 Myr) and the Local Association (t~50 Myr) moving groups. Unlike most past sub-mm studies, our sample was…

天体物理学 · 物理学 2009-11-10 Michael C. Liu , Brenda C. Matthews , Jonathan P. Williams , Paul G. Kalas

We have obtained mid-infrared spectra of nine cool-core galaxy clusters with the Infrared Spectrograph aboard the Spitzer Space Telescope. X-ray, ultraviolet and optical observations have demonstrated that each of these clusters hosts a…

宇宙学与河外天体物理 · 物理学 2009-08-25 G. E. de Messières , R. W. O'Connell , B. R. McNamara , M. Donahue , P. E. J. Nulsen , G. M. Voit , M. W. Wise

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…

We present new evidence for mature stellar populations with ages >100Myr in massive galaxies (M_stellar>10^10M_sun) seen at a time when the Universe was less than 1Gyr old. We analyse the prominent detections of two z~6 star-forming…

天体物理学 · 物理学 2009-11-10 Laurence Eyles , Andrew Bunker , Elizabeth Stanway , Mark Lacy , Richard Ellis , Michelle Doherty

Only 20\% of old field stars have detectable debris discs, leaving open the question of what disc, if any, is present around the remaining 80\%. Young moving groups allow to probe this population, since discs are expected to have been…

地球与行星天体物理 · 物理学 2021-02-10 Nicole Pawellek , Mark Wyatt , Luca Matrà , Grant Kennedy , Ben Yelverton

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 present ALMA observations of protoplanetary disks ("proplyds") in the Orion Nebula Cluster. We imaged 5 individual fields at 856um containing 22 HST-identified proplyds and detected 21 of them. Eight of those disks were detected for the…

Debris disks are extrasolar analogs to our own Kuiper Belt and they are detected around at least 17% of nearby Sun-like stars. The morphology and dynamics of a disk encode information about its history, as well as that of any exoplanets…

We present data obtained with the Infrared Array Camera (IRAC) aboard the Spitzer Space Telescope (Spitzer) for a sample of 74 young (t < 30 Myr old) Sun-like (0.7 < M(star)/M(Sun) < 1.5) stars. These are a sub-set of the observations that…

We present a Spitzer IRAC and MIPS survey of NGC 2451 A and B, two open clusters in the 50-80 Myr age range. We complement these data with extensive ground-based photometry and spectroscopy to identify the cluster members in the Spitzer…

太阳与恒星天体物理 · 物理学 2011-02-11 Zoltan Balog , Laszlo L. Kiss , Jozsef Vinko , G. H. Rieke , James Muzerolle , Andras Gaspar , Erick T. Young , Nadya Gorlova

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…

太阳与恒星天体物理 · 物理学 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

The thick disc contains stars formed within the first Gyr of Galactic history, and little is known about their planetary systems. The Spitzer MIPS instrument was used to search 11 of the closest of these old low-metal stars for…

太阳与恒星天体物理 · 物理学 2015-05-19 C. K. W. Sheehan , J. S. Greaves , G. Bryden , G. H. Rieke , K. Y. L. Su , M. C. Wyatt , C. A. Beichman

We present an analysis of Spitzer IRAC (3.6--8um) and MIPS (24um) imaging of members of the 16(+10/-5)Myr old open cluster NGC 1960 (M36). Models of terrestrial planet formation indicate that rocky planets are likely to achieve their final…

星系天体物理 · 物理学 2015-05-30 R. Smith , R. D. Jeffries