A 106 Day Period in the Nuclear Source X-8 in M33-Reference-Cited by-同舟云学术

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A 106 Day Period in the Nuclear Source X-8 in M33

Published:1997-11-20 Issue:1 Volume:490 Page:L47-L50
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:

Author:

Dubus Guillaume,Charles Philip A.,Long Knox S.,Hakala Pasi J.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference26 articles.

1. Variability analysis in low count rate sources

2. David, L. P., Harnden, F. R., Jr., Kearns, K. E. & Zombeck, M. V. 1996, The ROSAT HRI Calibration Report, U.S. ROSAT Science Data Center (Washington: Smithsonian Astrophys. Obs.)

3. Dubus, G., Charles, P. A., Long, K. S., Hakala, P. J. & Kuulkers, E. 1998, in preparation

4. A post-core-collapse model for the nucleus of M33

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1. Young Black Hole and Neutron Star Systems in the Nearby Star-forming Galaxy M33: The NuSTAR View;The Astrophysical Journal;2022-05-01

2. A New, Deep JVLA Radio Survey of M33;The Astrophysical Journal Supplement Series;2019-04-16

3. On the Nature of the X-Ray Emission from the Ultraluminous X-Ray Source, M33 X-8: New Constraints from NuSTAR and XMM-Newton;The Astrophysical Journal;2018-12-17

4. NuSTAR observations of the ultraluminous X-ray source M33 X-8: a black hole in a very high state?;Monthly Notices of the Royal Astronomical Society;2018-07-27

5. Swift-XRT six-year monitoring of the ultraluminous X-ray source M33 X-8;Astronomy & Astrophysics;2015-08

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