Talk:NGC 3199
Add topicLatest comment: 3 years ago by 76.119.40.77 in topic Reference summarized incorrectly
 | This article is rated Stub-class on Wikipedia's content assessment scale. It is of interest to the following WikiProjects: | |||||||||||||
| ||||||||||||||
.jpg){kind=small}
Reference summarized incorrectly
[edit]The journal article, "Hot Gas in the Wolf-Rayet Nebula NGC 3199"[1] starts with:
The Wolf-Rayet (WR) nebula NGC 3199 has been suggested to be a bow shock around its central star, WR 18, which is presumably a runaway star, because optical images of the nebula show a dominating arc of emission southwest of the star.
but it ends with:
... we conclude that WR 18 is not a runaway star and that the formation, chemical variations, and the shape of NGC 3199 depend on the initial configuration of the interstellar medium.
76.119.40.77 (talk) 09:12, 9 November 2022 (UTC) 76.119.40.77 (talk) 09:12, 9 November 2022 (UTC)
- I edited the article but do not know if I have accurately conveyed the correct information. 76.119.40.77 (talk) 09:30, 9 November 2022 (UTC)
References