Models for the Observable System Parameters of Ultraluminous X-ray Sources
We investigate the evolution of the properties of model populations of ultraluminous X-ray sources (ULXs) consisting of a black-hole accretor in a binary with a donor star. We have computed models corresponding to three different populations of black-hole binaries; two invoke stellar-mass (~10 Msun)...
Egile Nagusiak: | Madhusudhan, N, Rappaport, S, Podsiadlowski, P, Nelson, L |
---|---|
Formatua: | Journal article |
Argitaratua: |
IOP Publishing
2008
|
Antzeko izenburuak
-
MODELS FOR THE OBSERVABLE SYSTEM PARAMETERS OF ULTRALUMINOUS X-RAY SOURCES
nork: Madhusudhan, N, et al.
Argitaratua: (2008) -
Optical models for ultraluminous X-ray sources
nork: Madhusudhan, N, et al.
Argitaratua: (2008) -
Models of ultraluminous X-ray sources with intermediate-mass black holes
nork: Madhusudhan, N, et al.
Argitaratua: (2006) -
Models of ultraluminous X-ray sources with intermediate-mass black holes
nork: Madhusudhan, N, et al.
Argitaratua: (2006) -
ULTRALUMINOUS X-RAY SOURCES IN ARP 147
nork: Pooley, D., et al.
Argitaratua: (2015)