1998A&A...339L..45V


Query : 1998A&A...339L..45V

1998A&A...339L..45V - Astronomy and Astrophysics, volume 339, L45-48 (1998/11-2)

A second dust episode of the Wolf-Rayet system WR19: another long-period WC+O colliding-wind binary.

VEEN P.M., VAN DER HUCHT K.A., WILLIAMS P.M., CATCHPOLE R.M., DUIJSENS M.F.J., GLASS I.S. and SETIA GUNAWAN D.Y.A.

Abstract (from CDS):

We present observations of WR19 showing an infrared excess due to newly created dust similar to an event observed in 1988. We suggest that these episodes of dust-formation are periodic (P∼10yr) and related to the binary nature of the object, comparable to the colliding-wind binary WR140. In support of this thesis we identified absorption lines from a companion of spectral type O9.5-9.7. We propose monitoring the object to determine orbital parameters, non-thermal radio emission and the accurate shape of the infrared light-curve.

Abstract Copyright:

Journal keyword(s): stars: Wolf-Rayet - stars: individual: WR 19, HD 96620 - binaries: general - infrared: stars

Simbad objects: 8

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Number of rows : 8
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 * q Vel PM* 10 14 44.1556880397 -42 07 18.988830783 3.98 3.90 3.85 3.83 3.81 A2Va 136 0
2 WR 19 WR* 10 18 04.9885430688 -58 16 26.244521868   14.80 13.85     WC5+O9 68 0
3 HD 96220 ** 11 05 33.9808836888 -11 05 20.163039000   6.362 6.086     F0V 51 0
4 HD 96620 * 11 06 54.5858053512 -58 47 36.176175492   7.395 7.358 7.353 7.319 A0IV 38 0
5 HD 123008 s*b 14 07 30.6443226936 -64 28 08.781137868 8.58 10.00 9.50 9.44   ON9.2Iab 106 0
6 MR 93 WR* 19 28 15.6142522320 +19 33 21.527693100   14.83       WC7+O9(III) 110 0
7 HD 193793 WR* 20 20 27.9757908696 +43 51 16.286840244 6.90 7.25 6.85 4.58   WC7pd+O5.5fc 710 0
8 HD 195177 WR* 20 28 22.6636321896 +38 37 18.977440692 13.42 12.67 11.46     WC4+Be 88 0

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