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

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


Book ID
110849632
Publisher
John Wiley and Sons
Year
2011
Tongue
English
Weight
1023 KB
Volume
412
Category
Article
ISSN
0035-8711

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