THE GAS DYNAMICS OF NGC 4472 REVEALED BY XMM-NEWTON
We present results from a 100 ks XMM-Newton observation of the hot gas in the Virgo cluster elliptical galaxy NGC 4472. We find a surface brightness discontinuity ~21 kpc north of the nucleus, consistent with being a contact discontinuity between two moving fluids. We also detect a >60 kpc long r...
Κύριοι συγγραφείς: | , , , , , , , , |
---|---|
Άλλοι συγγραφείς: | |
Μορφή: | Άρθρο |
Γλώσσα: | en_US |
Έκδοση: |
IOP Publishing
2015
|
Διαθέσιμο Online: | http://hdl.handle.net/1721.1/95709 |