Exploring the unusually high black-hole-to-bulge mass ratios in NGC4342 and NGC4291: The asynchronous growth of bulges and black holes

Astrophysical Journal

Volumn 753, Issue 2, 2012, Pages

  Bogdán, Ákos ^a   Forman, William R ^a   Zhuravleva, Irina ^b   Mihos, J Christopher ^c   Kraft, Ralph P ^a   Harding, Paul ^c   Guo, Qi ^d,e   Li, Zhiyuan ^a   Churazov, Eugene ^b   Vikhlinin, Alexey ^a   Nulsen, Paul E J ^a   Schindler, Sabine ^f   Jones, Christine ^a  

^a SMITHSONIAN ASTROPHYSICAL OBSERVATORY   (United States)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^c CASE WESTERN RESERVE UNIVERSITY   (United States)

^d INSTITUTE OF GEOLOGY AND GEOPHYSICS   (China)

^e DURHAM UNIVERSITY   (United Kingdom)

^f UNIVERSITY OF INNSBRUCK   (Austria)

Author keywords

galaxies: bulges; galaxies: elliptical and lenticular, cD; galaxies: evolution; galaxies: individual (NGC 4291, NGC 4342); X rays: galaxies; X rays: ISM

Indexed keywords

EID: 84863098332     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/753/2/140     Document Type: Article

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