Probable intermediate-mass black holes in NGC 4559: XMM-Newton spectral and timing constraints
Open Access
- 21 March 2004
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 349 (1) , 39-51
- https://doi.org/10.1111/j.1365-2966.2004.07480.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 61 references indexed in Scilit:
- A Catalog of Candidate Intermediate‐Luminosity X‐Ray ObjectsThe Astrophysical Journal Supplement Series, 2002
- A Unified Description of the Timing Features of Accreting X‐Ray BinariesThe Astrophysical Journal, 2002
- Super-Eddington Fluxes from Thin Accretion Disks?The Astrophysical Journal, 2002
- The X-Ray Globular Cluster Population in NGC 1399The Astrophysical Journal, 2001
- Black hole masses from power density spectra: determinations and consequencesMonthly Notices of the Royal Astronomical Society, 2001
- The Nature of Accreting Black Holes in Nearby Galaxy NucleiThe Astrophysical Journal, 1999
- Do the Spectra of Soft X‐Ray Transients Reveal Bulk‐Motion Inflow Phenomenon?The Astrophysical Journal, 1999
- The FIRST Survey: Faint Images of the Radio Sky at Twenty CentimetersThe Astrophysical Journal, 1995
- Abundances of the elements: Meteoritic and solarGeochimica et Cosmochimica Acta, 1989
- Luminosity Indicators in the Spectra of Quasi-Stellar ObjectsThe Astrophysical Journal, 1977