Radio and Millimeter Observations of YSOs

Details Radio and Millimeter Observations of YSOs Radio and Millimeter Observations of YSOs

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hia....15..258r&link_type=abstract

Highlights of Astronomy, Volume 15, p. 258-260

Astronomy and Astrophysics

Astronomy

Stars: Formation, Ism: Individual (Iras 16547-4247)

Scientific paper

The growth of a forming star takes place by accretion from the surrounding dense medium, facilitated by a circumstellar disk. But at the same time the forming system produces collimated outflows of gas that remove excess angular momentum and magnetic flux. A key question in the field is whether we can extend the disk/jet model to stars of the largest masses or if other ingredients are present. In this note, I review recent observations from the Very Large Array and the Submillimeter Array, of IRAS 16547-4247, a massive young stellar object that exhibits evidence for both a disk and an outflow.

Affiliated with

Also associated with

No associations

Rating

Radio and Millimeter Observations of YSOs does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Radio and Millimeter Observations of YSOs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio and Millimeter Observations of YSOs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1484583