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| Query : 2019RNAAS...3..146J |
2019RNAAS...3..146J - Research Notes of the AAS, 3, 146 (2019/October-0)
A Comparison of the Well-constrained Geometry of V444 Cygni and Two Possible Analogs: WR 21 and WR 62a.
JOHNSON R.A., FULLARD A.G., LOMAX J.R., COOPER K., LEON-ALVAREZ D., HOFFMAN J.L. and NORDSIECK K.H.
Journal keyword(s): Wolf-Rayet stars - Close binary stars - Massive stars - Spectropolarimetry
Simbad objects: 3
| Number of rows : 3 |
| 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 | HD 90657 | WR* | 10 26 31.4087563344 | -58 38 26.182481568 | 9.53 | 10.07 | 9.65 | 9.84 | WN5+O4-6 | 169 | 0 | |
| 2 | WR 62a | WR* | 14 32 37.6995368616 | -61 29 54.128039280 | 14.491 | 13.056 | 12.687 | 11.147 | WN5+O5.5/6 | 13 | 0 | |
| 3 | HD 193576 | WR* | 20 19 32.4229160448 | +38 43 53.959035756 | 8.15 | 8.53 | 8.00 | WN5+O6II-V | 721 | 0 |
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