Abstract
Recent RXTE observations have identified a very high state for several black hole candidates. Kubota et al. (2001, 2004) reported that this state can be accounted for by the inverse Compton scattering and slim disk emission. This idea is important for the purpose of obtaining a unified view of disk emission around black holes, but the sample is still poor. In addition, it has not been confirmed that the idea can be effectively applied to black hole binaries that repeat outbursts. For this reason, we analyzed the black hole candidate 4U1630-47, which is known to exhibit X-ray outbursts with a period of about 650 days, and we found it to be in a very high state in the outburst of 1998. We also found a very high state in the outburst of 1996. By considering inverse Compton scattering and slim disk emission, we found that these two very high states can be accounted as proposal by Kubota et al. It is found that 4U1630-47 is the third to exhibit three states. Three states are thought to be common among black hole binaries.
| Original language | English |
|---|---|
| Pages (from-to) | 303-304 |
| Number of pages | 2 |
| Journal | Progress of Theoretical Physics Supplement |
| Volume | 155 |
| Publication status | Published - 2004 |
| Externally published | Yes |
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- Physics and Astronomy(all)
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Three spectral states of the disk X-ray emission of the black hole candidate 4U1630-47. / Abe, Yukiko; Fukazawa, Yasushi; Kubota, Aya.
In: Progress of Theoretical Physics Supplement, Vol. 155, 2004, p. 303-304.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - Three spectral states of the disk X-ray emission of the black hole candidate 4U1630-47
AU - Abe, Yukiko
AU - Fukazawa, Yasushi
AU - Kubota, Aya
PY - 2004
Y1 - 2004
N2 - Recent RXTE observations have identified a very high state for several black hole candidates. Kubota et al. (2001, 2004) reported that this state can be accounted for by the inverse Compton scattering and slim disk emission. This idea is important for the purpose of obtaining a unified view of disk emission around black holes, but the sample is still poor. In addition, it has not been confirmed that the idea can be effectively applied to black hole binaries that repeat outbursts. For this reason, we analyzed the black hole candidate 4U1630-47, which is known to exhibit X-ray outbursts with a period of about 650 days, and we found it to be in a very high state in the outburst of 1998. We also found a very high state in the outburst of 1996. By considering inverse Compton scattering and slim disk emission, we found that these two very high states can be accounted as proposal by Kubota et al. It is found that 4U1630-47 is the third to exhibit three states. Three states are thought to be common among black hole binaries.
AB - Recent RXTE observations have identified a very high state for several black hole candidates. Kubota et al. (2001, 2004) reported that this state can be accounted for by the inverse Compton scattering and slim disk emission. This idea is important for the purpose of obtaining a unified view of disk emission around black holes, but the sample is still poor. In addition, it has not been confirmed that the idea can be effectively applied to black hole binaries that repeat outbursts. For this reason, we analyzed the black hole candidate 4U1630-47, which is known to exhibit X-ray outbursts with a period of about 650 days, and we found it to be in a very high state in the outburst of 1998. We also found a very high state in the outburst of 1996. By considering inverse Compton scattering and slim disk emission, we found that these two very high states can be accounted as proposal by Kubota et al. It is found that 4U1630-47 is the third to exhibit three states. Three states are thought to be common among black hole binaries.
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UR - http://www.scopus.com/inward/citedby.url?scp=11044226088&partnerID=8YFLogxK
M3 - Article
AN - SCOPUS:11044226088
VL - 155
SP - 303
EP - 304
JO - Progress of Theoretical Physics
JF - Progress of Theoretical Physics
SN - 0033-068X
ER -