Interaction between AGB Wind and Nova Outburst: The Case of V407 Cyg, a Symbiotic Star

Details Interaction between AGB Wind and Nova Outburst: The Case of V407 Cyg, a Symbiotic Star Interaction between AGB Wind and Nova Outburst: The Case of V407 Cyg, a Symbiotic Star

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aspc..445..319d&link_type=abstract

Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants. Proceedings of a conference held at University Ca

Astronomy and Astrophysics

Astronomy

Scientific paper

We report on the time variation of SiO maser emission from the symbiotic star V407 Cyg after the classical nova outburst with concurrent γ-ray emission in 2010 March. The SiO J=1-0, v=2 line at 42.821 GHz has been detectable persistently, but the line profile exhibited a dramatic change two weeks after the outburst. A new persistent component appeared at the lower velocity side in the spectrum three weeks later. The observation indicates that the SiO emitting regions were terminated in a time-scale of two weeks by the hot wind of the nova, but the region was replenished quickly by cool molecular gases expelled from the mira, possibly through the first Lagrangian point of the binary system.

Affiliated with

Also associated with

No associations

Rating

Interaction between AGB Wind and Nova Outburst: The Case of V407 Cyg, a Symbiotic Star 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 Interaction between AGB Wind and Nova Outburst: The Case of V407 Cyg, a Symbiotic Star, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interaction between AGB Wind and Nova Outburst: The Case of V407 Cyg, a Symbiotic Star will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-829040