ОписаниеDevelopment of massive elliptical galaxies.jpg
English: This graphic shows the evolutionary sequence in the growth of massive elliptical galaxies over 13 billion years, as gleaned from space-based and ground-based telescopic observations. The growth of this class of galaxies is quickly driven by rapid star formation and mergers with other galaxies.
This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use. The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org. For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.
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Название изображения
This graphic shows the evolutionary sequence in the growth of massive elliptical galaxies over 13 billion years, as gleaned from space-based and ground-based telescopic observations. The growth of this class of galaxies is quickly driven by rapid star formation and mergers with other galaxies. Link NASA Press release
Источник
ESA/Hubble
Поставщик, кто предоставил изображение
NASA, ESA, and S. Toft (Niels Bohr Institute) Illustration Credit: NASA, ESA, S. Toft (Niels Bohr Institute), and A. Feild (STScI) Science Credit: NASA, ESA, S. Toft (Niels Bohr Institute), V. Smolcic (University of Zagreb), B. Magnelli (Argelander Institute for Astronomy), A. Karim (Argelander Institute for Astronomy and Durham University), A. Zirm (Niels Bohr Institute), M. Michalowski (University of Edinburgh and Universiteit Gent), P. Capak (California Institute of Technology), K. Sheth (National Radio Astronomy Observatory), K. Schawinski (ETH Zurich), J.-K. Krogager (Niels Bohr Institute and European Southern Observatory), S. Wuyts (Max Planck Institute for Extraterrestrial Physics), D. Sanders (University of Hawaii), A. Man (Niels Bohr Institute), D. Lutz (Max Planck Institute for Extraterrestrial Physics), J. Staguhn (NASA Goddard Space Flight Center and Johns Hopkins University), S. Berta (Max Planck Institute for Extraterrestrial Physics), H. McCracken (Institut d'Astrophysique de Paris), J. Krpan (University of Zagreb), D. Riechers (Cornell University and California Institute of Technology), and G. Brammer (European Southern Observatory and STScI)