Radio emission and absorption regions in SS 433

Details Radio emission and absorption regions in SS 433 Radio emission and absorption regions in SS 433

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998newar..42..641p&link_type=abstract

New Astronomy Reviews, Volume 42, Issue 9-10, p. 641-643.

Astronomy and Astrophysics

Astronomy

5

Stars: Individual (Ss433), Ism: Jets And Outflows, Radio Continuum: Stars Copyright: (C) 1998 Elsevier Science B.V. All Rights Reserved.

Scientific paper

We present multi-frequency VLBI observations of SS 433 at 1.6, 5, and 15 GHz. The central region of the source is resolved and shows a double core-wing structure with a central gap, resolvable only at high frequency. Spectral properties of these components indicate that free-free absorption occurs, but only towards the innermost part of the jets. We have also discovered an extended emission region which is nearly perpendicular to the twin jets and has a steep spectrum. Possibly, our observations indicate the presence of a large, flattened structure in the equatorial plane of the system.

Affiliated with

Also associated with

No associations

Rating

Radio emission and absorption regions in SS 433 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 emission and absorption regions in SS 433, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio emission and absorption regions in SS 433 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-763497