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相关论文: Spitzer Far-Infrared Detections of Cold Circumstel…

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We present a survey of mid-infrared gas-phase lines toward a sample of 76 circumstellar disks around low mass pre-main sequence stars from the Spitzer "Cores to Disks" legacy program. We report the first detections of [Ne II] and [Fe I]…

(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

Micron size extrasolar dust particles have been convincingly detected by satellites. Larger extrasolar meteoroids (5-35 microns) have most likely been detected by ground based radar at Arecibo and New Zealand. We present estimates of the…

天体物理学 · 物理学 2009-11-10 Norman Murray , Joe Weingartner , Paul Capobianco

By comparing sensitive Spitzer Space Telescope (SST) infrared and Green Bank Telescope 21 cm observations, we are able to report the first detection of dust emission in Complex C, the largest High Velocity Cloud in the sky. Dust in the…

天体物理学 · 物理学 2009-11-11 M. -A. Miville-Deschenes , F. Boulanger , W. T. Reach , A. Noreiga-Crespo

We have searched for evidence of emission at 15 microns with ISOCAM and at 90 microns with ISOPHOT from dust orbiting six nearby pulsars, both in binaries and in isolation, located at distances between about 100 to 1000 pc. No emission was…

天体物理学 · 物理学 2009-11-07 Lydie Koch-Miramond , Martin Haas , Eric Pantin , Philipp Podsiadlowski , Tim Naylor , Marc Sauvage

A powerful way to observe directly the solid state inventory of dense molecular clouds is by infrared spectroscopy of background stars. We present Spitzer/IRS 5-20 micron spectra of ices toward stars behind the Serpens and Taurus molecular…

We present unpublished Spitzer IRAC observations of the HH 1/2 young stellar outflow processed with a high angular resolution deconvolution algorithm that produces sub-arcsecond (approx. 0.6" - 0.8") images. In the resulting mid-infrared…

太阳与恒星天体物理 · 物理学 2015-06-04 A. Noriega-Crespo , A. C. Raga

(abridged) We determine the disk mass distribution around 336 stars in the young Orion Nebula cluster by imaging a 2.5' x 2.5' region in 3 mm continuum emission with the Owens Valley Millimeter Array. For this sample of 336 stars, we…

天体物理学 · 物理学 2009-11-11 J. A. Eisner , John M. Carpenter

We present new Spitzer Space Telescope observations of stars in the young ~5 Myr gamma Velorum stellar cluster. Combining optical and 2MASS photometry, we have selected 579 stars as candidate members of the cluster. With the addition of the…

天体物理学 · 物理学 2009-11-13 Jesus Hernandez , Lee Hartmann , Nuria Calvet , R. D. Jeffries , R. Gutermuth , J. Muzerolle , J. Stauffer

Debris discs are known to exist around many planet-host stars, but no debris dust has been found so far in systems with transiting planets. Using publicly available catalogues, we searched for infrared excesses in such systems. In the…

地球与行星天体物理 · 物理学 2015-05-30 Alexander V. Krivov , Martin Reidemeister , Simone Fiedler , Torsten Löhne , Ralph Neuhäuser

We present mid-infrared Spitzer Space Telescope observations of a complete sample of star-forming dwarf galaxies selected from the KPNO International Spectroscopic Survey. The galaxies span a wide range in mid-infrared properties. Contrary…

天体物理学 · 物理学 2009-11-13 J. L. Rosenberg , M. L. N. Ashby , J. J. Salzer , J. -S. Huang

The Solar System gas giants are each surrounded by many moons, with at least 50 prograde satellites thought to have formed from circumplanetary material. Just like the Sun is not the only star surrounded by planets, extrasolar gas giants…

地球与行星天体物理 · 物理学 2019-07-17 Sebastián Pérez , Sebastián Marino , Simon Casassus , Clément Baruteau , Alice Zurlo , Christian Flores , Gael Chauvin

We present IRAC/MIPS Spitzer observations of intermediate-mass stars in the 5 Myr old Lambda Orionis cluster. In a representative sample of stars earlier than F5 (29 stars), we find a population of 9 stars with a varying degree of moderate…

太阳与恒星天体物理 · 物理学 2014-11-20 Jesús Hernández , Nuria Calvet , L. Hartmann , J. Muzerolle , R. Gutermuth , J. Stauffer

We describe results from a survey for J=3-2 12CO emission from visible stars with an infrared excess. The line is clearly detected in 21 objects, with molecular gas (>10^-3 Jupiter masses) common in targets with infrared excesses >0.01…

天体物理学 · 物理学 2009-11-10 W. R. F. Dent , J. S. Greaves , I. M. Coulson

We report the detection of an excess in dust continuum emission at 233~GHz (1.3~mm in wavelength) in the protoplanetary disk around TW~Hya revealed through high-sensitivity observations at $\sim$3~au resolution with the Atacama Large…

Since 2003, the Spitzer Space Telescope has provided groundbreaking views of Galactic star formation in bands from 3.6 past 24 microns. During the cryogenic mission (the first 5.5 years), variability of young stars at these bands was noted,…

太阳与恒星天体物理 · 物理学 2015-03-18 L. M. Rebull

We report results of a re-analysis of archival Spitzer IRAC direct imaging surveys encompassing a variety of nearby stars. Our sample is generated from the combined observations of 73 young stars (median age, distance, spectral type = 85…

地球与行星天体物理 · 物理学 2016-06-22 Stephen Durkan , Markus Janson , Joseph Carson

We have identified 17 A-type stars in the Galactic Plane that have mid-IR excesses at 8 micron. From the observed colors in the (r'-H_alpha)-(r'-i') plane, we first identified 23050 early A-type main sequence (MS) star candidates in the…

A set of six debris disk candidates identified with IRAS or WISE excesses were observed at either 350 um or 450 um with the CSO. Five of the targets - HIP 51658, HIP 68160, HIP 73512, HIP 76375, and HIP 112460 - have among the largest…

太阳与恒星天体物理 · 物理学 2015-06-16 J. Bulger , T. Hufford , A. Schneider , J. Patience , I. Song , R. J. De Rosa , A. Rajan , C. D. Dowell , D. McCarthy , C. Kulesa

Supernova fallback disks around neutron stars have been discussed to influence the evolution of the diverse neutron star populations. Slowly rotating neutron stars are most promising to find such disks. Searching for the cold and warm…

太阳与恒星天体物理 · 物理学 2015-06-22 B. Posselt , G. G. Pavlov , S. B. Popov , S. Wachter
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