Ram pressure stripping in high-density environments
Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure stripping, ie the pressure exerted by the …
affect their evolution. Among these, ram pressure stripping, ie the pressure exerted by the …
On the origin of the faint-end of the red sequence in high-density environments
A Boselli, G Gavazzi - The Astronomy and Astrophysics Review, 2014 - Springer
With the advent of the new generation wide-field cameras it became possible to survey in an
unbiased mode galaxies spanning a variety of local densities, from the core of rich clusters …
unbiased mode galaxies spanning a variety of local densities, from the core of rich clusters …
The next generation Virgo cluster survey (NGVS). I. Introduction to the survey
L Ferrarese, P Cote, JC Cuillandre… - The Astrophysical …, 2012 - iopscience.iop.org
THE NEXT GENERATION VIRGO CLUSTER SURVEY (NGVS). I. INTRODUCTION TO THE
SURVEY - IOPscience Skip to content IOP Science home Accessibility Help Search Journals …
SURVEY - IOPscience Skip to content IOP Science home Accessibility Help Search Journals …
GASP. IX. Jellyfish galaxies in phase-space: an orbital study of intense ram-pressure stripping in clusters
YL Jaffé, BM Poggianti, A Moretti… - Monthly Notices of …, 2018 - academic.oup.com
It is well known that galaxies falling into clusters can experience gas stripping due to ram
pressure by the intra-cluster medium. The most spectacular examples are galaxies with …
pressure by the intra-cluster medium. The most spectacular examples are galaxies with …
A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE)-I. Introduction to the survey
A Boselli, M Fossati, L Ferrarese, S Boissier… - Astronomy & …, 2018 - aanda.org
The Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) is a blind narrow-
band (NB) Hα+[NII] imaging survey carried out with MegaCam at the Canada–France …
band (NB) Hα+[NII] imaging survey carried out with MegaCam at the Canada–France …
The Burrell Schmidt deep Virgo survey: tidal debris, galaxy halos, and diffuse intracluster light in the Virgo cluster
JC Mihos, P Harding, JJ Feldmeier… - The Astrophysical …, 2016 - iopscience.iop.org
We present the results of a deep imaging survey of the Virgo cluster of galaxies,
concentrated around the cores of Virgo subclusters A and B. The goal of this survey was to …
concentrated around the cores of Virgo subclusters A and B. The goal of this survey was to …
Cold gas properties of the Herschel Reference Survey-II. Molecular and total gas scaling relations
We study the properties of the cold gas component of the interstellar medium of the Herschel
Reference Survey, a complete volume-limited (15≲ D≲ 25 Mpc), K-band-selected sample of …
Reference Survey, a complete volume-limited (15≲ D≲ 25 Mpc), K-band-selected sample of …
[HTML][HTML] The resolved scaling relations in DustPedia: Zooming in on the local Universe
V Casasola, S Bianchi, L Magrini, AV Mosenkov… - Astronomy & …, 2022 - aanda.org
Aims. We perform a homogeneous analysis of an unprecedented set of spatially resolved
scaling relations (SRs) between interstellar medium (ISM) components, that is to say dust …
scaling relations (SRs) between interstellar medium (ISM) components, that is to say dust …
Cold gas properties of the Herschel Reference Survey-III. Molecular gas stripping in cluster galaxies
The Herschel Reference Survey is a complete volume-limited, K-band-selected sample of
nearby objects including Virgo cluster and isolated objects. Using a recent compilation of Hi …
nearby objects including Virgo cluster and isolated objects. Using a recent compilation of Hi …
The effect of the environment on the H i scaling relations
L Cortese, B Catinella, S Boissier… - Monthly Notices of the …, 2011 - academic.oup.com
We use a volume-, magnitude-limited sample of nearby galaxies to investigate the effect of
the environment on the H i scaling relations. We confirm that the H i-to-stellar mass ratio …
the environment on the H i scaling relations. We confirm that the H i-to-stellar mass ratio …