The Radial Orbits of Ram-pressure-stripped Galaxies in Clusters from the GASP Survey

We analyze a sample of 244 ram-pressure-stripped candidate galaxy members within the virial radius of 62 nearby clusters to determine their velocity anisotropy profile β ( r ). We use previously determined mass profiles for the 62 clusters to build an ensemble cluster by stacking the 62 cluster samp...

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Main Authors: Andrea Biviano, Bianca M. Poggianti, Yara Jaffé, Ana C. Lourenço, Lorenzo Pizzuti, Alessia Moretti, Benedetta Vulcani
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad2c09
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author Andrea Biviano
Bianca M. Poggianti
Yara Jaffé
Ana C. Lourenço
Lorenzo Pizzuti
Alessia Moretti
Benedetta Vulcani
author_facet Andrea Biviano
Bianca M. Poggianti
Yara Jaffé
Ana C. Lourenço
Lorenzo Pizzuti
Alessia Moretti
Benedetta Vulcani
author_sort Andrea Biviano
collection DOAJ
description We analyze a sample of 244 ram-pressure-stripped candidate galaxy members within the virial radius of 62 nearby clusters to determine their velocity anisotropy profile β ( r ). We use previously determined mass profiles for the 62 clusters to build an ensemble cluster by stacking the 62 cluster samples in projected phase space. We solve the Jeans equation for dynamical equilibrium by two methods, MAMPOSSt and the Jeans inversion technique, and determine β ( r ) both in parametric form and nonparametrically. The two methods consistently indicate that the orbits of the ram-pressure-stripped candidates are increasingly radial with distance from the cluster center, from almost isotropic ( β ≃ 0) at the center, to very radial at the virial radius ( β ≃ 0.7). The orbits of cluster galaxies undergoing ram pressure stripping are similar to those of spiral cluster galaxies but more radially elongated at large radii.
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spelling doaj.art-3a7c78c8e7d54e7080be85235bee42412024-04-12T08:10:20ZengIOP PublishingThe Astrophysical Journal1538-43572024-01-01965211710.3847/1538-4357/ad2c09The Radial Orbits of Ram-pressure-stripped Galaxies in Clusters from the GASP SurveyAndrea Biviano0https://orcid.org/0000-0002-0857-0732Bianca M. Poggianti1https://orcid.org/0000-0001-8751-8360Yara Jaffé2https://orcid.org/0000-0003-2150-1130Ana C. Lourenço3https://orcid.org/0000-0002-4393-7798Lorenzo Pizzuti4https://orcid.org/0000-0001-5654-7580Alessia Moretti5https://orcid.org/0000-0002-1688-482XBenedetta Vulcani6https://orcid.org/0000-0003-0980-1499INAF-Osservatorio Astronomico di Trieste , via G.B. Tiepolo 11, 34143 Trieste, Italy; IFPU-Institute for Fundamental Physics of the Universe , via Beirut 2, 34014 Trieste, ItalyINAF-Osservatorio Astronomico di Padova , Vicolo Osservatorio 5, I-35122 Padova, ItalyDepartamento de Física, Universidad Técnica Federico Santa María , Avenida España 1680, Valparaíso, Chile; Instituto de Física y Astronomía, Universidad de Valparaíso , Avenida Gran Bretaña 1111, Valparaíso, ChileInstituto de Física y Astronomía, Universidad de Valparaíso , Avenida Gran Bretaña 1111, Valparaíso, Chile; European Southern Observatory (ESO) , Alonso de Cordova 3107, Santiago, ChileDipartimento di Fisica G. Occhialini, Universitá degli Studi di Milano Bicocca , Piazza della Scienza 3, I-20126 Milano, ItalyINAF-Osservatorio Astronomico di Padova , Vicolo Osservatorio 5, I-35122 Padova, ItalyINAF-Osservatorio Astronomico di Padova , Vicolo Osservatorio 5, I-35122 Padova, ItalyWe analyze a sample of 244 ram-pressure-stripped candidate galaxy members within the virial radius of 62 nearby clusters to determine their velocity anisotropy profile β ( r ). We use previously determined mass profiles for the 62 clusters to build an ensemble cluster by stacking the 62 cluster samples in projected phase space. We solve the Jeans equation for dynamical equilibrium by two methods, MAMPOSSt and the Jeans inversion technique, and determine β ( r ) both in parametric form and nonparametrically. The two methods consistently indicate that the orbits of the ram-pressure-stripped candidates are increasingly radial with distance from the cluster center, from almost isotropic ( β ≃ 0) at the center, to very radial at the virial radius ( β ≃ 0.7). The orbits of cluster galaxies undergoing ram pressure stripping are similar to those of spiral cluster galaxies but more radially elongated at large radii.https://doi.org/10.3847/1538-4357/ad2c09Galaxy clustersGalaxy kinematicsGalaxy evolutionRam pressure stripped tails
spellingShingle Andrea Biviano
Bianca M. Poggianti
Yara Jaffé
Ana C. Lourenço
Lorenzo Pizzuti
Alessia Moretti
Benedetta Vulcani
The Radial Orbits of Ram-pressure-stripped Galaxies in Clusters from the GASP Survey
The Astrophysical Journal
Galaxy clusters
Galaxy kinematics
Galaxy evolution
Ram pressure stripped tails
title The Radial Orbits of Ram-pressure-stripped Galaxies in Clusters from the GASP Survey
title_full The Radial Orbits of Ram-pressure-stripped Galaxies in Clusters from the GASP Survey
title_fullStr The Radial Orbits of Ram-pressure-stripped Galaxies in Clusters from the GASP Survey
title_full_unstemmed The Radial Orbits of Ram-pressure-stripped Galaxies in Clusters from the GASP Survey
title_short The Radial Orbits of Ram-pressure-stripped Galaxies in Clusters from the GASP Survey
title_sort radial orbits of ram pressure stripped galaxies in clusters from the gasp survey
topic Galaxy clusters
Galaxy kinematics
Galaxy evolution
Ram pressure stripped tails
url https://doi.org/10.3847/1538-4357/ad2c09
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