572 citations · 4.5k across the 82 of their papers we have counts for
7 papers · 2 filters
Giant Molecular Clouds in the Local Group Galaxy M33
P. Gratier, J. Braine, N. J. Rodriguez-Fernandez +7
We present an analysis of the systematic CO(2-1) survey at 12" resolution covering most of the local group spiral M 33 which, at a distance of 840 kpc, is close enough that individ…
The Herschel Virgo Cluster Survey - VIII. The Bright Galaxy Sample
J. I. Davies, S. Bianchi, L. Cortese +20
We describe the Herschel Virgo Cluster Survey (HeViCS) and the first data that cover the complete survey area (four 4 x 4 deg2 regions). We use these data to measure and compare th…
The population of Young Stellar Clusters throughout the disk of M33
Saurabh Sharma, Edvige Corbelli, Carlo Giovanardi +2
The properties of young stellar clusters (YSCs) in M33, identified from the center out to about twice the size of the bright star-forming disk,are investigated. We find 915 discret…
The Herschel Virgo Cluster Survey. IX. Dust-to-gas mass ratio and metallicity gradients in four Virgo spiral galaxies
Laura Magrini, Simone Bianchi, Edvige Corbelli +20
Using Herschel data from the Open Time Key Project the Herschel Virgo Cluster Survey (HeViCS), we investigated the relationship between the metallicity gradients expressed by metal…
Stellar structures in the outer regions of M33
M. Grossi, N. Hwang, E. Corbelli +3
We present Subaru/Suprime-Cam deep V and I imaging of seven fields in the outer regions of M33. Our aim is to search for stellar structures corresponding to extended HI clouds foun…
The CO-to-H2 Conversion Factor From Infrared Dust Emission Across the Local Group
Adam K. Leroy, Alberto Bolatto, Karl Gordon +8
We estimate the conversion factor relating CO emission to H2 mass, alpha_CO, in five Local Group galaxies that span approximately an order of magnitude in metallicity - M31, M 33,…
On the nature of faint mid-infrared sources in M33
Edvige Corbelli, Carlo Giovanardi, Francesco Palla +1
We investigate the nature of 24micron sources in M33 which have weak or no associated Halpha emission. Both bright evolved stars and embedded star forming regions are visible as co…