IRAS 18153-1651: an H ii region with a possible wind bubble blown by a young main-sequence B star
We report the results of spectroscopic observations and numerical modelling of the H ii region IRAS 18153−1651. Our study was motivated by the discovery of an optical arc and two main-sequence stars of spectral type B1 and B3 near the centre of IRAS 18153−1651. We interpret the arc as the edge of th...
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| Main Authors: | , |
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| Format: | Article (Journal) |
| Language: | English |
| Published: |
14 December 2016
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2017, Volume: 466, Issue: 2, Pages: 1857-1867 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stw3257 |
| Online Access: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stw3257 Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/466/2/1857/2687809/IRAS-18153-1651-an-H-ii-region-with-a-possible 
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| Author Notes: | V.V. Gvaramadze, J. Mackey, A.Y. Kniazev, N. Langer, A.-N. Chené, N. Castro, T.J. Haworth and E.K. Grebel |
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IRAS 18153-1651: an H II region with a possible wind bubble blown by a young main-sequence B star
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