Displacement of X-ray sources from star clusters in starburst galaxies
Open Access
- 21 February 2004
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 348 (2) , L28-L32
- https://doi.org/10.1111/j.1365-2966.2004.07516.x
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This publication has 40 references indexed in Scilit:
- Star cluster formation and disruption time-scales -- II. Evolution of the star cluster system in the fossil starburst of M82Monthly Notices of the Royal Astronomical Society, 2003
- The [F[CLC]e[/CLC] [CSC]ii[/CSC]] 1.644 Micron Emission in M82 and NGC 253: Is It a Measure of the Supernova Rate?The Astronomical Journal, 2003
- The Time-variable Ultraluminous X-Ray Sources of “The Antennae”The Astrophysical Journal, 2003
- The Fossil Starburst in M82The Astronomical Journal, 2001
- Hot Plasma and Black Hole Binaries in Starburst Galaxy M82Science, 2000
- TheHubble Space TelescopeKey Project on the Extragalactic Distance Scale. XXV. A Recalibration of Cepheid Distances to Type Ia Supernovae and the Value of the Hubble ConstantThe Astrophysical Journal, 2000
- Dust and Recent Star Formation in the Core of NGC 5253The Astronomical Journal, 1997
- The Central Star Cluster of the Star-forming Dwarf Galaxy NGC 5253The Astrophysical Journal, 1996
- Enhanced winds and tidal streams in massive X-ray binariesThe Astrophysical Journal, 1991
- X Rays From Normal GalaxiesAnnual Review of Astronomy and Astrophysics, 1989