activity
19942026
most citedUBVRI Light Curves of 44 Type Ia Supernovae

372 citations · 6.9k across the 115 of their papers we have counts for

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Showing 2019 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2019

Radio Recombination Line Observations Toward the Massive Star Forming Region W51 IRS1

Mishaal. I. Jan, D. Anish Roshi, M. E. Lebrón +6

We observed radio recombination lines (RRLs) toward the W51 molecular cloud complex, one of the most active star forming regions in our Galaxy. The UV radiation from young massive…

astro-ph.GA2019★ 27 cited

Mass Assembly of Stellar Systems and their Evolution with the SMA (MASSES) -- Full Data Release

Ian W. Stephens, Tyler L. Bourke, Michael M. Dunham +13

We present and release the full dataset for the Mass Assembly of Stellar Systems and their Evolution with the SMA (MASSES) survey. This survey used the Submillimeter Array (SMA) to…

astro-ph.GA2019★ 52 cited

An Episodic Wide-angle Outflow in HH 46/47

Yichen Zhang, Hector G. Arce, Diego Mardones +7

During star formation, the accretion disk drives fast MHD winds which usually contain two components, a collimated jet and a radially distributed wide-angle wind. These winds entra…

astro-ph.GA2019★ 49 cited

Widespread Molecular Outflows in the Infrared Dark Cloud G28.37+0.07: Indications of Orthogonal Outflow-Filament Alignment

Shuo Kong, Héctor G. Arce, María José Maureira +3

We present ALMA CO(2-1) observations toward a massive infrared dark cloud G28.37+0.07. The ALMA data reveal numerous molecular (CO) outflows with a wide range of sizes throughout t…

astro-ph.GA2019★ 8 cited

The CARMA-NRO Orion Survey: Statistical Signatures of Feedback in the Orion A Molecular Cloud

Jesse R. Feddersen, Héctor G. Arce, Shuo Kong +2

We investigate the relationship between turbulence and feedback in the Orion A molecular cloud using maps of CO(1-0), CO(1-0) and CO(1-0) from the CARMA-NRO Or…

astro-ph.GA2019★ 70 cited

The CARMA-NRO Orion Survey: The filamentary structure as seen in CO emission

S. T. Suri, A. Sanchez-Monge, P. Schilke +18

We present an initial overview of the filamentary structure in the Orion A molecular cloud utilizing a high angular and velocity resolution CO(1-0) emission map that was rec…