Direct Observations of Bipolar Outflow from HM Sagittae

Details Direct Observations of Bipolar Outflow from HM Sagittae Direct Observations of Bipolar Outflow from HM Sagittae

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..457e&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 457-458

Astronomy and Astrophysics

Astrophysics

Binaries: Symbiotic, Radio Continuum: Stars, Stars: Individual: Hm Sge

Scientific paper

We observed HM Sagittae with theMulti-Element Radio Linked
Interferometer Network (MERLIN) at 6 cm and 18cm. We find non-thermal
bipolar outflow in the eastwest direction, associated with optical
emission lines, and thermal ridges to the north and south associated
with the UV nebulosity detected by the HST.

Affiliated with

Also associated with

No associations

Rating

Direct Observations of Bipolar Outflow from HM Sagittae 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 Direct Observations of Bipolar Outflow from HM Sagittae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Direct Observations of Bipolar Outflow from HM Sagittae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1630263