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Galaxy Evolution and Feedback across Different Environments (IAU S359)

Galaxy Evolution and Feedback across Different Environments (IAU S359)

Galaxy Evolution and Feedback across Different Environments (IAU S359)

Thaisa Storchi Bergmann, Universidade Federal do Rio Grande do Sul, Brazil
William Foreman, Harvard-Smithsonian Center for Astrophysics
Roderik Overzier, Observatório Nacional, Rio de Janeiro
Rogério Riffel, Universidade Federal do Rio Grande do Sul, Brazil
May 2021
Available
Hardback
9781108490689
£102.00
GBP
Hardback

    The goal of IAU Symposium 359 on 'Galaxy Evolution and Feedback across Different Environments' (GALFEED) was to bring together the active galactic nuclei (AGN) and galaxy evolution scientific communities. The AGN phase occurs in most galaxies and critically influences their evolution, so it is important to study the two processes together and for researchers, in both topics, to learn from one another. They ask key questions such as: How do galaxies acquire their gas and how efficiently is it transformed into stars? How is the supermassive black hole in a galaxy center fuelled to become an AGN? What is the main physical mechanism that quenches star formation? How powerful are the stellar and AGN feedback processes in regulating galaxy evolution? And what is the role of the environment on galaxy evolution and AGN triggering? Astronomers engage in these discussions spanning from early galaxies to the present day.

    • Brings together the AGN and galaxy evolution science communities, that usually attend separate specialized meetings
    • Covers discussions of a broad range of topics from galaxy formation to the present-day Universe, over 6 topical sessions
    • One of the last scientific Symposia to gather in-person in 2020, before the cancellations due to COVID-19

    Reviews & endorsements

    '… this is certainly worth looking at in your library …' Steve Phillipps, The Observatory

    See more reviews

    Product details

    May 2021
    Hardback
    9781108490689
    524 pages
    254 × 182 × 23 mm
    0.98kg
    Available

    Table of Contents

    • 1. Formation and Early Growth of Galaxies and SMBHs Roderik Overzier
    • 2. Cosmic Noon Cristina Furlanetto and Sebastian Sanchez
    • 3. Evolution of Galaxies and AGN in High-Density Environments from High to Low Redshifts João Steiner and William Forman
    • 4. Secular Evolution and Internal Processes: Mass Quenching, Stellar and AGN Feedback over Different Z's Tiago Ricci and Marina Trevisan
    • 5. Secular Evolution and Internal Processes: Mechanisms for Fueling Star Formation and AGN Thaisa Storchi Bergmann and Daniel Ruschel Dutra
    • 6. The Present-Day Universe: Spatially Resolved Studies of Stellar and Gas Content, Excitation and Metallicity Ana Chies Santos
    • 7: Discussion – Questions and Answers.
      Contributors
    • Andrew Newman, Rainer Weinberger, Karin Menendez-Delmestre, Laurie Riguccini, Ezequiel Treister, Carlos Gómez-Guijarro, Kristina Nyland, Dillon Dong, Pallavi Patil, Mark Lacy, Amy Kimball, Gregg Hallinan, Sumit Sarbadhicary, Emil Polisensky, Namir Kassim, Wendy Peters, Tracy Clarke, Dipanjan Mukherjee, Sjoert Van Velzen, Vincenzo Mainieri, Michael Brotherton, Jaya Maithil, Adam Myers, Ohad Shemmer, Brandon Matthews, Cooper Dix, Pu Du, Jian-Min Wang, Carlo Cannarozzo, Carlo Nipoti, Alessandro Sonnenfeld, Alexie Leauthaud, Song Huang, Benedikt Diemer, Grecco Oyarzún, Maximilien Franco, Luigi Spinoglio, Juan Fernández Ontiveros, Sabrina Mordini, Andrey Vayner, Shelley Wright, Norm Murray, Lee Armus, Anna Boehle, Maren Cosens, James Larkin, Etsuko Mieda, Gregory Walth, Clare Wethers, Nischal Acharya, Jari Kotilainen, Roberto De Propris, Malte Schramm, Andreas Schulze, Martin Hardcastle, Christine Jones, William Forman, Bianca Poggianti, Anderson Caproni, Gustavo Lanfranchi, Akos Bogdan, Ralph Kraft, Eugene Churazov, Scott Randall, Ming Sun, Ewan O'Sullivan, Jan Vrtilek, Paul Nulsen, Kei Ito, Steve Kraemer, T. Jane Turner, D. Michael Crenshaw, Henrique Schmitt, Mitchell Revalski, Travis Fischer, Minju Lee, Ichi Tanaka, Ryohei Kawabe, Bunyo Hatsukade, Kodama Tadayuki, Kotaro Kohno, Kouichiro Nakanishi, Toshiki Saito, Ken-ichi Tadaki, Yoichi Tamura, Filippo Maccagni, Paolo Serra, Matteo Murgia, Federica Govoni, Kana Morokuma-Matsui, Dane Kleiner, Fernanda Roman de Oliveira, Ana Chies Santos, Fabrício Ferrari, Geferson Lucatelli, Henrique Schmitt, Nathan Secrest, Laura Blecha, Barry Rothberg, Jackeline Fischer, Damien Spérone-Longin, Christopher Harrison, Stephen Molyneux, Jan Scholtz, Miranda Jarvis, Giacomo Venturi, Alessandro Marconi, Alberto Rodríguez-Ardila, Marcos Faria, Richard Davies, Dalya Baron, Taro Shimizu, Hagai Netzer, Mar Mezcua, Raffaella Morganti, Tom Oosterloo, Clive Tadhunter, Daniel Ruschel-Dutra, Thaisa Storchi-Bergmann, Allan Schnorr-Müller, Keiichi Wada, Anelise Audibert, Francoise Combes, Santiago García-Burillo, Kalliopi Dasyra, D. Michael Crenshaw, Matilde Mingozzi, Giovanni Cresci, Giacomo Venturi, Alessandro Marconi, Filippo Mannucci, Rodrigo Nemmen, Roberta Duarte, Joao Navarro, Sandra Raimundo, Natalia Vale Asari, Grazyna Stasinska, Michael Beasley, Ryan Leaman, Ignacio Trujillo, Mireia Montes Quiles, Alexandre Vazdekis, Nuria Salvador Rusiñol, Elham Eftekhari, Anna Ferré-Mateu, Ignacio Martín-Navarro, Lucimara Martins, Sebastian F. Sanchez, Carlos Lopez Coba, Grazyna Stasinska, Dorota Wierzbowska, João Steiner, Roberto Menezes, Tiago Ricci, Alexandre Vazdekis, Pablo Rogdríguez-Beltrán, Miguel Cerviño, Michael Beasley

    • Editors
    • Thaisa Storchi Bergmann , Universidade Federal do Rio Grande do Sul, Brazil
    • William Foreman , Harvard-Smithsonian Center for Astrophysics
    • Roderik Overzier , Observatório Nacional, Rio de Janeiro
    • Rogério Riffel , Universidade Federal do Rio Grande do Sul, Brazil