The episodic dust-making Wolf-Rayet star HD 38030 in the Large Magellanic Cloud

被引:4
|
作者
Williams, Peredur M. [1 ]
Morrell, Nidia, I [2 ]
Boutsia, Konstantina [2 ]
Massey, Philip [3 ,4 ]
机构
[1] Univ Edinburgh, Inst Astron, Royal Observ, Edinburgh EH9 3HJ, Midlothian, Scotland
[2] Carnegie Observ, Las Campanas Observ, Casilla 601, La Serena, Chile
[3] Lowell Observ, 1400 W Mars Hill Rd, Flagstaff, AZ 86011 USA
[4] No Arizona Univ, Dept Astron & Planetary Sci, Flagstaff, AZ 86011 USA
基金
美国国家航空航天局;
关键词
binaries: spectroscopic; circumstellar matter; stars: individual: HD 38030; stars: winds; stars: Wolf-Rayet; INFRARED-SURVEY-EXPLORER; X-RAY; PHOTOMETRY; STELLAR; NEOWISE; EMISSION; CATALOG; GRAINS; DENIS; WINDS;
D O I
10.1093/mnras/stab1625
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Mid-infrared photometry of the Wolf-Rayet star HD 38030 in the Large Magellanic Cloud from the NEOWISE-R mission show it to have undergone a dust-formation episode in 2018 and the dust to have cooled in 2019-20. New spectroscopy with the MagE spectrograph on the Magellan I Baade Telescope in 2019 and 2020 show absorption lines attributable to a companion of type near O9.7III-IV. We found a significant shift in the radial velocity of the C IV lambda lambda 5801-12 blend compared with the RVs measured in 1984 and 1993. The results combine to suggest that HD 38030 is a colliding-wind binary having short-lived dust formation episodes, like the Galactic systems WR 140 and WR 19, but at intervals in excess of 20 yr.
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页码:5029 / 5037
页数:9
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