Formation of intermediate-mass black holes in circumnuclear regions of galaxies
この論文をさがす
抄録
application/pdf
Recent high-resolution X-ray imaging studies have discovered possible candidates of intermediate-mass black holes with masses of $M_\bullet \sim 10^{2-4} \MO$ in circumnuclear regions of many (disk) galaxies. It is known that a large number of massive stars are formed in a circumnuclear giant H {\sc ii} region. Therefore, we propose that continual merger of compact remnants left from these massive stars is responsible for the formation of such an intermediate-mass black hole within a timescale of $\sim 10^9$ years. A necessary condition is that several hundreds of massive stars are formed in a compact region with a radius of a few pc.
収録刊行物
-
- Publications of the Astronomical Society of Japan
-
Publications of the Astronomical Society of Japan 52 (3), 533-537, 2000-02
Tokyo : Astronomical Society of Japan
- Tweet
詳細情報 詳細情報について
-
- CRID
- 1050001338928162048
-
- NII論文ID
- 10004678497
-
- NII書誌ID
- AA1082896X
-
- ISSN
- 00046264
-
- NDL書誌ID
- 5434023
-
- 本文言語コード
- en
-
- 資料種別
- journal article
-
- データソース種別
-
- IRDB
- NDL
- CiNii Articles