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Query : 2019A&A...622L...3E |
2019A&A...622L...3E - Astronomy and Astrophysics, volume 622, L3-3 (2019/2-1)
Wind Roche lobe overflow in high-mass X-ray binaries. A possible mass-transfer mechanism for ultraluminous X-ray sources.
EL MELLAH I., SUNDQVIST J.O. and KEPPENS R.
Abstract (from CDS):
Abstract Copyright: © ESO 2019
Journal keyword(s): X-rays: binaries - accretion - accretion disks - stars: black holes - supergiants - stars: winds - outflows - stars: neutron
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 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | CXOU J002029.1+591651 | HXB | 00 20 29.09 | +59 16 51.9 | ~ | 170 | 0 | |||||
2 | CXOU J005510.0-374212 | HXB | 00 55 09.990 | -37 42 12.16 | 22.44 | WNE | 126 | 1 | ||||
3 | V* GP Vel | HXB | 09 02 06.8608812864 | -40 33 16.899168060 | 6.85 | 7.37 | 6.87 | 6.31 | 6.05 | B0.5Ia | 1505 | 0 |
4 | [JRW2005b] 122 | UX? | 14 03 32.38 | +54 21 03.0 | 21.13 | ~ | 113 | 0 | ||||
5 | NAME NGC 7793 P13 | ULX | 23 57 50.90 | -32 37 26.6 | ~ | 190 | 0 |
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