60 citations · 208 across the 8 of their papers we have counts for
8 papers
CO(2-1) Survey at 9 parsec resolution in the SMC
H. P. Saldaño, M. Rubio, A. D. Bolatto +3
The Small Magellanic Cloud (SMC) is the closest low-metallicity galaxy to the Milky Way where the dynamical state of molecular clouds can be analyzed. We present a CO(2-1) survey a…
First Detection of the Molecular Cloud Population in the Extended Ultraviolet (XUV) Disk of M83
Jin Koda, Linda Watson, Francoise Combes +8
We report a CO(3-2) detection of 23 molecular clouds in the extended ultraviolet (XUV) disk of the spiral galaxy M83 with ALMA. The observed 1kpc^2 region is at about 1.24 times th…
ALMA resolves molecular clouds in the metal poor Magellanic Bridge A
M. T. Valdivia-Mena, M. Rubio, A. D. Bolatto +2
(Abridged)We characterize gas and dust emission in Magellanic Bridge A, which has the highest 870m excess of emission found in single dish surveys. Using the ALMA telescope, we…
Stochastic modeling of the time variability of ALMA calibrators
A. E. Guzmán, C. Verdugo, H. Nagai +5
Characterizing the variability of the extragalactic sources used for calibration in the Atacama Large Millimeter/Sub-millimeter Array (ALMA) is key to assess the flux scale uncerta…
ALMA CO(2-1) observations in the XUV disk of M83
Isadora C. Bicalho, Francoise Combes, Monica Rubio +2
The extended ultraviolet (XUV) disk galaxies are one of the most interesting objects studied in the last few years. The UV emission, revealed by GALEX, extends well beyond the opti…
First Results from the and ALMA Spectroscopic Surveys of the SMC: The Relationship Between [CII]-bright Gas and CO-bright Gas at Low Metallicity
Katherine E. Jameson, Alberto D. Bolatto, Mark Wolfire +15
The Small Magellanic Cloud (SMC) provides the only laboratory to study the structure of molecular gas at high resolution and low metallicity. We present results from the Herschel S…
Ram Pressure Stripping in the Virgo Cluster
Celia Verdugo, Françoise Combes, Kalliopi Dasyra +2
Gas can be violently stripped from their galaxy disks in rich clusters, and be dispersed over 100kpc-scale tails or plumes. Young stars have been observed in these tails, suggestin…
Carbon Monoxide Clouds at Low-Metallicity in the WLM Galaxy
Bruce G. Elmegreen, Monica Rubio, Deidre A. Hunter +3
Carbon monoxide (CO) is the primary tracer for interstellar clouds where stars form, yet CO has never been detected in galaxies with an Oxygen abundance relative to Hydrogen less t…