411 citations · 2.4k across the 26 of their papers we have counts for
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The Spitzer Survey of Interstellar Clouds in the Gould Belt. VI. The Auriga-California Molecular Cloud observed with IRAC and MIPS
Hannah Broekhoven-Fiene, Brenda C. Matthews, Paul M. Harvey +15
We present observations of the Auriga-California Molecular Cloud (AMC) at 3.6, 4.5, 5.8, 8.0, 24, 70 and 160 micron observed with the IRAC and MIPS detectors as part of the Spitzer…
A First Look at the Auriga-California Giant Molecular Cloud With Herschel and the CSO: Census of the Young Stellar Objects and the Dense Gas
Paul M. Harvey, Cassandra Fallscheer, Adam Ginsburg +7
We have mapped the Auriga/California molecular cloud with the Herschel PACS and SPIRE cameras and the Bolocam 1.1 mm camera on the Caltech Submillimeter Observatory (CSO) with the…
YSOVAR: Six pre-main-sequence eclipsing binaries in the Orion Nebula Cluster
M. Morales-Calderón, J. R. Stauffer, K. G. Stassun +17
Eclipsing binaries (EBs) provide critical laboratories for empirically testing predictions of theoretical models of stellar structure and evolution. Pre-main-sequence (PMS) EBs are…
The Spitzer Survey of Interstellar Clouds in the Gould Belt. V. Ophiuchus North Observed with IRAC and MIPS
Jennifer Hatchell, Susan Terebey, Tracy Huard +10
We present Spitzer IRAC (2.1 sq. deg.) and MIPS (6.5 sq. deg.) observations of star formation in the Ophiuchus North molecular clouds. This fragmentary cloud complex lies on the ed…
The Mass Distributions of Starless and Protostellar Cores in Gould Belt Clouds
S. I. Sadavoy, J. Di Francesco, S. Bontemps +12
Using data from the SCUBA Legacy Catalogue (850 um) and Spitzer Space Telescope (3.6 - 70 um), we explore dense cores in the Ophiuchus, Taurus, Perseus, Serpens, and Orion molecula…
Evolutionary Signatures in the Formation of Low-Mass Protostars. II. Towards Reconciling Models and Observations
Michael M. Dunham, Neal J. Evans, Susan Terebey +2
A long-standing problem in low-mass star formation is the "luminosity problem," whereby protostars are underluminous compared to the accretion luminosity expected both from theoret…
The Dust Emissivity Spectral Index in the Starless Core TMC-1C
Scott Schnee, Melissa Enoch, Alberto Noriega-Crespo +10
In this paper we present a dust emission map of the starless core TMC-1C taken at 2100 microns. Along with maps at 160, 450, 850 and 1200 microns, we study the dust emissivity spec…