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19952023
most citedYoung Stellar Objects in the Gould Belt

303 citations · 6.9k across the 133 of their papers we have counts for

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Showing 2015Show all

11 papers · 1 filter

astro-ph.SR2015★ 46 cited

The JCMT Gould Belt Survey: A First Look at Dense Cores in Orion B

H. Kirk, J. Di Francesco, D. Johnstone +54

We present a first look at the SCUBA-2 observations of three sub-regions of the Orion B molecular cloud: LDN 1622, NGC 2023/2024, and NGC 2068/2071, from the JCMT Gould Belt Legacy…

astro-ph.EP2015★ 17 cited

IR-excesses around nearby Lambda Boo stars are caused by debris disks rather than ISM bow waves

Zachary H Draper, Brenda C Matthews, Grant M Kennedy +3

Lambda Boo stars are predominately A-type stars with solar abundant C, N, O, and S, but up to 2 dex underabundances of refractory elements. The stars' unusual surface abundances co…

astro-ph.EP2015

Direct imaging of an asymmetric debris disk in the HD 106906 planetary system

Paul G. Kalas, Abhijith Rajan, Jason J. Wang +53

We present the first scattered light detections of the HD 106906 debris disk using Gemini/GPI in the infrared and HST/ACS in the optical. HD 106906 is a 13 Myr old F5V star in the…

astro-ph.SR2015★ 50 cited

The AU Mic Debris Disk: far-infrared and submillimeter resolved imaging

Brenda C. Matthews, Grant Kennedy, Bruce Sibthorpe +20

We present far-infrared and submillimeter maps from the Herschel Space Observatory and the James Clerk Maxwell Telescope of the debris disk host star AU Microscopii. Disk emission…

astro-ph.GA2015★ 303 cited

Young Stellar Objects in the Gould Belt

Michael M. Dunham, Lori E. Allen, Neal J. Evans +14

We present the full catalog of Young Stellar Objects (YSOs) identified in the 18 molecular clouds surveyed by the Spitzer Space Telescope "cores to disks" (c2d) and "Gould Belt" (G…

astro-ph.GA2015★ 21 cited

ALMA Observations of the Largest Proto-Planetary Disk in the Orion Nebula, 114-426: A CO Silhouette

John Bally, Rita K. Mann, Josh Eisner +7

We present ALMA observations of the largest protoplanetary disk in the Orion Nebula, 114-426. Detectable 345 GHz (856 micron) dust continuum is produced only in the 350 AU central…