Galaxy stellar mass functions of different morphological types in clusters, and their evolution between z= 0.8 and 0-Reference-Cited by-同舟云学术

Galaxy stellar mass functions of different morphological types in clusters, and their evolution between z= 0.8 and 0

Published:2011-02-05 Issue:1 Volume:412 Page:246-268
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Vulcani Benedetta,Poggianti Bianca M.,Aragón-Salamanca Alfonso,Fasano Giovanni,Rudnick Gregory,Valentinuzzi Tiziano,Dressler Alan,Bettoni Daniela,Cava Antonio,D'Onofrio Mauro,Fritz Jacopo,Moretti Alessia,Omizzolo Alessandro,Varela Jesús

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/412/1/246/3077885/mnras0412-0246.pdf

Reference99 articles.

1. The buildup of stellar mass and the 3.6μm luminosity function in clusters fromz = 1.25 toz = 0.2

2. Evidence for systematic evolution in the properties of galaxies in distant clusters

3. Quantifying the Bimodal Color‐Magnitude Distribution of Galaxies

4. Galaxy bimodality versus stellar mass and environment

Cited by 98 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. A morphological analysis of the galaxy cluster XLSSC 122 at z = 1.98;Monthly Notices of the Royal Astronomical Society;2024-08-15

2. Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology;The Astrophysical Journal;2024-04-29

3. GALAXY CRUISE: Spiral and ring classifications for bright galaxies at z = 0.01–0.3;Publications of the Astronomical Society of Japan;2024-01-29

4. Post-processing of galaxies due to major cluster mergers;Astronomy & Astrophysics;2023-12

5. Distinct distributions of elliptical and disk galaxies across the Local Supercluster as a ΛCDM prediction;Nature Astronomy;2023-11-20