Measuring the black hole mass in ultraluminous X-ray sources with the X-ray scaling method
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/473/1/136/21282525/stx2178.pdf
Reference71 articles.
1. An ultraluminous X-ray source powered by an accreting neutron star
2. The recurrent ultra-luminous X-ray transient NGC 253 ULX1
3. A 33 hour period for the Wolf-Rayet/black hole X-ray binary candidate NGC 300 X-1
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1. Broadband X-Ray Spectral Analysis of the ULX NGC 1313 X-1 Using JeTCAF: Origin of the ULX Bubble;Publications of the Astronomical Society of the Pacific;2023-05-01
2. Estimating black hole masses in obscured AGN using X-rays;Monthly Notices of the Royal Astronomical Society;2021-01-22
3. Revisiting the long term X-ray spectral evolution of Seyfert 1 galaxies;Monthly Notices of the Royal Astronomical Society;2019-11-18
4. ULX contribution to stellar feedback: an intermediate-mass black hole candidate and the population of ULXs in the low-metallicity starburst galaxy ESO 338-4;Astronomy & Astrophysics;2019-07
5. Are narrow-line Seyfert 1 galaxies highly accreting low-MBH AGNs?;Monthly Notices of the Royal Astronomical Society;2018-07-11
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