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| Query : 2017PASJ...69...92K |
2017PASJ...69...92K - Publ. Astron. Soc. Jap., 69, 92 (2017)
Theoretical modeling of Comptonized X-ray spectra of super-Eddington accretion flow: Origin of hard excess in ultraluminous X-ray sources.
KITAKI T., MINESHIGE S., OHSUGA K. and KAWASHIMA T.
Journal keyword(s):
Simbad objects: 4
| Number of rows : 4 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | [SST2011] J081929.00+704219.3 | ULX | 08 19 28.99 | +70 42 19.4 | ~ | 213 | 2 | |||||
| 2 | [KCF2005] M82 G | ULX | 09 55 51.040 | +69 40 45.49 | ~ | 284 | 1 | |||||
| 3 | NAME NGC 5907 ULX | ULX | 15 15 58.60 | +56 18 10.0 | ~ | 180 | 0 | |||||
| 4 | NAME NGC 7793 P13 | ULX | 23 57 50.90 | -32 37 26.6 | ~ | 225 | 0 |
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