Molecular gas in normal late-type galaxies ?

By A. Boselli, J. Lequeux, G. Gavazzi. 2002

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View Paper: https://www.semanticscholar.org/paper/0f409ce6eac46e6862192523a1e483e100e30351

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In Astronomy and Astrophysics

Citations in the corpus

The Origin of Dwarf Ellipticals in the Virgo Cluster (2008, background): “…and past star formation activity (Gavazzi et al. 1991, 1998, 2002b, 2006a), the atomic (Gavazzi et al. 2005b, 2006b) and molecular gas content (Boselli 1994; Boselli et al. 1994, 1997a, 2002), the radio continuum and IR properties of cluster galaxies (Gavazzi & Boselli 1999; Gavazzi et al. 1991).”
Star Formation from Galaxies to Globules (2001, methodology): “…total galactic star formation rate is really proportional to the first power of the total gas mass, as suggested by studies that find a constant efficiency (see x 2.3), then we should use an observed rate given by SFR volume = ð14Þ for constant gas consumption time 109:6 yr (Boselli et al. 2002).”
THE IMPACT OF INTERACTIONS, BARS, BULGES, AND ACTIVE GALACTIC NUCLEI ON STAR FORMATION EFFICIENCY IN LOCAL MASSIVE GALAXIES (2012, methodology): “Based on a sample of galaxies for which independent measures of αCO are available (Boselli et al. 2002), we choose a value of S60µm/S100µm = 0.5 as the threshold to determine αCO (Gracia-Carpio et al., in preparation).”
The dust scaling relations of the Herschel Reference Survey (2012, background): “3 can be seen as the result of the variation of SSFR with stellar mass (e.g., Boselli et al. 2001; Schiminovich et al. 2007).”
REGULARITY UNDERLYING COMPLEXITY: A REDSHIFT-INDEPENDENT DESCRIPTION OF THE CONTINUOUS VARIATION OF GALAXY-SCALE MOLECULAR GAS PROPERTIES IN THE MASS-STAR FORMATION RATE PLANE (2013, unknown): “…et al. (2012) subsequently were able to show that the conversion factor of high-z MS galaxies scales with gas-phase metallicity in a similar manner as the negative power laws observed for local galaxies (e.g., Wilson 1995, Israel 1997, Boselli et al. 2002, Leroy et al. 2011, Schruba et al. 2012).”
Environmental Effects on Late‐Type Galaxies in Nearby Clusters (2006, methodology): “The H i surface density correlates tightly with the H i deficiency parameter (Boselli et al. 2002).”
CO Molecular Gas in Infrared-luminous Galaxies (2003, unknown): “The mean ratio M(H2)/M(H i) is substantially larger than that found for optically selected latetype galaxies (0.15) by Boselli et al. (2002).”