期刊
ASTROPHYSICAL JOURNAL
卷 758, 期 2, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/758/2/85
关键词
accretion, accretion disks; black hole physics; galaxies: individual (NGC 247); X-rays: binaries
资金
- National Natural Science Foundation of China [10903004, 10978001, 11222327]
- 973 Program of China [2009CB824800]
- Foundation for the Author of National Excellent Doctoral Dissertation of China [200935]
- Tsinghua University Initiative Scientific Research Program
- Program for New Century Excellent Talents in University
- STScI grant [HST-GO-12375.01-A]
- Chandra grant [GO1-12048X]
We report on multiwavelength observations of the supersoft ultraluminous X-ray source (ULX) in NGC 247 made with the Chandra X-Ray Observatory and Hubble Space Telescope. We aligned the X-ray and optical images using three objects present on both and identified a unique, point-like optical counterpart to the ULX. The X-ray to optical spectrum is well fitted with an irradiated disk model if the extinction measured for Cepheids in NGC 247 is used. Assuming only Galactic extinction, the spectrum can be modeled as a standard thin accretion disk. Either result leads to the conclusion that a disk interpretation of the X-ray spectrum is valid, thus the source may be in the X-ray thermal state and contain an intermediate-mass black hole of at least 600 M-circle dot. In contrast to other supersoft ULXs that are transient and exhibit a luminosity temperature relation inconsistent with a disk interpretation of the X-ray emission, the NGC 247 ULX has a relatively steady flux and all available X-ray data are consistent with emission from a disk in the thermal state.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据