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| Query : 2021PASJ...73..630K |
2021PASJ...73..630K - Publ. Astron. Soc. Jap., 73, 630-638 (2021)
What determines the unique spectra of super-Eddington accretors? Origin of optically thick and low-temperature coronae in super-Eddington accretion flows.
KAWANAKA N. and MINESHIGE S.
Journal keyword(s):
Simbad objects: 5
| Number of rows : 5 |
| 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] J034555.61+680455.3 | ULX | 03 45 55.612 | +68 04 55.29 | ~ | 176 | 1 | |||||
| 2 | RX J123551+27561 | ULX | 12 35 51.71 | +27 56 04.1 | ~ | 79 | 1 | |||||
| 3 | [FK2005] 23 | ULX | 13 29 38.62 | +58 25 05.6 | ~ | 134 | 2 | |||||
| 4 | [FK2005] 25 | ULX | 14 03 19.63 | -41 22 58.7 | ~ | 252 | 0 | |||||
| 5 | Granat 1915+105 | HXB | 19 15 11.55576 | +10 56 44.9052 | ~ | 2810 | 0 |
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