2004A&A...420L...9R


Query : 2004A&A...420L...9R

2004A&A...420L...9R - Astronomy and Astrophysics, volume 420L9-13 (2004/6-3)

WR20a: A massive cornerstone binary system comprising two extreme early-type stars.

RAUW G., DE BECKER M., NAZE Y., CROWTHER P.A., GOSSET E., SANA H., VAN DER HUCHT K.A., VREUX J.-M. and WILLIAMS P.M.

Abstract (from CDS):

We analyse spectroscopic observations of WR20a revealing that this star is a massive early-type binary system with a most probable orbital period of ∼3.675days. Our spectra indicate that both components are most likely of WN6ha or O3If*/WN6ha spectral type. The orbital solution for a period of 3.675days yields extremely large minimum masses of 70.7±4.0 and 68.8 ±3.8M☉ for the two stars. These properties make WR20a a cornerstone system for the study of massive star evolution.

Abstract Copyright: ∼

Journal keyword(s): binaries: spectroscopic - stars: early-type - stars: fundamental parameters - stars: individual: WR 20a

CDS comments: Mk 42 = Cl* NGC 2070 MEL 42.

Simbad objects: 10

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Number of rows : 10
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 [HSH95] 38 ** 05 38 42.0996 -69 06 07.795           O3V+O6V 25 0
2 Brey 77 WR* 05 38 42.1044150840 -69 05 55.335965424     12.86   12.79 O2If* 90 0
3 [HSH95] 42 ** 05 38 42.1802 -69 06 02.384           O3V+O3V 17 0
4 V* V712 Car EB* 10 23 58.0126366512 -57 45 48.937268268 15.466 15.473 13.5 12.6   O3If*/WN6+O3If*/WN6 176 0
5 Cl Westerlund 2 OpC 10 23 58.1 -57 45 49           ~ 400 0
6 GUM 29 HII 10 24 14.6 -57 46 58           ~ 219 0
7 HD 92740 WR* 10 41 17.5158425712 -59 40 36.895992960 5.68 6.50 6.42 7.38   WN7h+O9III-V 426 0
8 NGC 3603 OpC 11 14 57.9 -61 14 32           ~ 1136 1
9 Cl* NGC 3603 MDS C WR* 11 15 07.5851367565 -61 15 38.027795970   12.94 11.89     WN6h 49 0
10 HD 214419 WR* 22 36 53.9548302648 +56 54 20.989190232 8.68 9.376 8.996 8.962   WN6o+O9Ib/II 385 1

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