X‐Ray Emission from a Merger Remnant, NGC 7252 (the “Atoms‐for‐Peace” Galaxy)
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/567/i=2/a=892/pdf
Reference27 articles.
1. Far‐Infrared Emission From E and E/S0 Galaxies
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1. Diffuse X-Ray-emitting Gas in Major Mergers;The Astronomical Journal;2018-01-23
2. THE [O III] NEBULA OF THE MERGER REMNANT NGC 7252: A LIKELY FAINT IONIZATION ECHO;The Astrophysical Journal;2013-08-05
3. XMM-Newtonobservations of the merger-remnant galaxies NGC 3921 and 7252;Monthly Notices of the Royal Astronomical Society;2004-09
4. AHubble Space TelescopeWFPC2 Investigation of the Nuclear Morphology in the Toomre Sequence of Merging Galaxies;The Astronomical Journal;2003-12
5. ChandraObservations of the Interacting NGC 4410 Galaxy Group;The Astronomical Journal;2003-10
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