The central regions of galaxies show the presence of super massive black holes and/or very dense stellar clusters. Both such objects seem to follow similar host-galaxy correlations, suggesting that they are members of the same family of Compact Massive Objects. Here we investigate a huge data collection of Compact Massive Objects properties to correlate them with absolute magnitude, velocity dispersion and mass of their host galaxies. We draw also some preliminary astrophysical conclusion
Scaling Correlations Amoung Central Massive Objects and Their Host Galaxies / TOSTA E MELO, Iara; CAPUZZO DOLCETTA, Roberto Angelo. - In: JOURNAL OF PHYSICS. CONFERENCE SERIES. - ISSN 1742-6588. - ELETTRONICO. - 689:1(2016). (Intervento presentato al convegno 6th Young Researcher Meeting, L’Aquila 2015 tenutosi a Gran Sasso Science Institute (GSSI)L'Aquila; Italy) [10.1088/1742-6596/689/1/012008].
Scaling Correlations Amoung Central Massive Objects and Their Host Galaxies
TOSTA E MELO, IARA;CAPUZZO DOLCETTA, Roberto Angelo
2016
Abstract
The central regions of galaxies show the presence of super massive black holes and/or very dense stellar clusters. Both such objects seem to follow similar host-galaxy correlations, suggesting that they are members of the same family of Compact Massive Objects. Here we investigate a huge data collection of Compact Massive Objects properties to correlate them with absolute magnitude, velocity dispersion and mass of their host galaxies. We draw also some preliminary astrophysical conclusion| File | Dimensione | Formato | |
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