MERLIN observations of bipolar outflow from HM Sagittae

Details MERLIN observations of bipolar outflow from HM Sagittae MERLIN observations of bipolar outflow from HM Sagittae

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995yera.conf....4e&link_type=abstract

The XXVIIth Young European Radio Astronomers Conference, ed. D.A. Green and W. Steffen, in association with Cambridge University

Astronomy and Astrophysics

Astronomy

Scientific paper

MERLIN maps of HM Sagittae at 6 cm and 18 cm wavelengths are presented. At 6 cm, the inner nebula has been mapped at a resolution of 60 milli-arcsec, revealing two parallel ridge structures to the north and south of a deep central minimum. In addition, these central features are surrounded by a complex, weak structure. The ridges and many of the weak features are correlated with ultra-violet (UV) structure observed with the Hubble Space Telescope (HST). The 18 cm map reveals elongated structure to the east and west of the star's position. There is strong evidence that the east and west edges of this extension are non-thermal. The E-W and N-S features are associated with components detected with optical spectroscopy. The radial velocities of these components suggest that the E-W features are a high velocity bipolar outflow.

Affiliated with

Also associated with

No associations

Rating

MERLIN 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 MERLIN 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 MERLIN observations of bipolar outflow from HM Sagittae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-852913