Light-Curve of a Hot Spot on Advection-Like Accretion Disk(Poster) :
Bibliographic Information
- Other Title
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- Light-Curve of a Hot Spot on Advection-Like Accretion Disk
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Abstract
Light curves of a hot spot rotating in a relativistic Keplerian disk were found to be periodic with typically two peaks, originating from a gravitational focusing effect and a Doppler boost. On the other hand, we found that light curves of a hot spot spirally infalling in a sub-Keplerian advective disk are aperiodic with typically a single peak, originating from a gravitational focusing effect or a Doppler boost. Such a difference in light curves of a hot spot can discriminate background disk models.
Journal
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- Progress of Theoretical Physics Supplement
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Progress of Theoretical Physics Supplement 155 329-330, 2004
Oxford University Press (OUP)
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Details 詳細情報について
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- CRID
- 1360566396831170432
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- NII Article ID
- 110001216400
- 210000127839
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- NII Book ID
- AA00791466
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- ISSN
- 03759687
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- Data Source
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- Crossref
- NDL-Digital
- CiNii Articles