2017
DOI: 10.1017/s1743921317009565 View full text |Buy / Rent full text
|
|

Abstract: The detection of hydrogen radio-recombination maser lines (RRLs) toward MWC349A in the year 1989 opened the chance to place constraints on the kinematics of an ionized circumstellar disk around a massive star. Since then, a significant number of observations have allowed improving our understanding of this source to the point that we have established that its ionized wind launching occurs at a distance of ~24 au as claimed by disk wind models. On the other hand, this field of study has undergone considerable d… Show more

Help me understand this report

Search citation statements

Order By: Relevance
0
0
0
0
0
0
0
0

Publication Types

Select...

Relationship

0
0

Authors

Journals