TheHerschelVirgo Cluster Survey

2011/06/06 by L. Magrini, Laura Magrini, S. Bianchi +42 · 3 citations
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Cluster (spacecraft) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Physics #Stellar, planetary, and galactic studies #Virgo Cluster #astro-ph.CO

paper · pdf · doi:10.1051/0004-6361/201116872

13 pages, 8 figures, A&A accepted

arxiv created 2011/06/06 · openalex publication_date 2011/06/10 · arxiv updated 2015/05/28 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. 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 abundances in the gas phase as traced by the chemical composition of HII regions, and in the solid phase, as traced by the dust-to-gas mass ratio.

Citations

• VLA IMAGING OF VIRGO SPIRALS IN ATOMIC GAS (VIVA). I. THE ATLAS AND THE H I PROPERTIES
• Oxygen abundances in dwarf irregular galaxies and the metallicity-luminosity relationship
• [O iii]/[N ii] as an abundance indicator at high redshift
• Using Strong Lines to Estimate Abundances in Extragalactic H ii Regions and Starburst Galaxies
• CI and CO in the center of M 51
• The distribution of cosmic-ray sources in the Galaxy, γ-rays and the gradient in the CO-to-H2relation
• The Resolved Properties of Extragalactic Giant Molecular Clouds
• The Chemical Composition of the Sun

Cited by

• The Herschel Exploitation of Local Galaxy Andromeda (HELGA). IV. Dust scaling relations at sub-kpc resolution
• The DiskMass Survey
• Cosmic evolution of molecular gas mass density from an empirical relationship between L1.4 GHz and L′CO

Related

• Open clusters in the Gaia-ESO Survey tracing the chemical history of the Milky Way
• Open clusters as key tracers of Galactic chemical evolution
• On the metallicity of open clusters. III. Homogenised sample
• A Global Census of Metals in the Universe
• Measuring Chemical Abundances in Extragalactic Metal-Rich HII Regions