Multiwavelength Observations of V1494 AQL in Outburst

Details Multiwavelength Observations of V1494 AQL in Outburst Multiwavelength Observations of V1494 AQL in Outburst

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cxo..prop..798s&link_type=abstract

Chandra Proposal ID #03300850

Computer Science

Chandra Proposal Id #03300850

Scientific paper

We propose 2 HRC-S+LETG followup observations of V1494 Aql which we observed with CHANDRA as a TOO in Cycle 1. Our grating data show that it has become a Super Soft Source (SSS) and an analysis of the light curve shows a 2500s period. More grating data is necessary both to determine its evolution during the SSS phase and to measure any changes in period. We also observed a factor of 6 rise in counts during the observation and further data could help to determine if this were a common phenomenon. It is evolving slowly in the optical and should still be bright in X-rays in Cycle 3. Analysis of the grating data will allow us to study the composition of the ejecta, the lifetime of the TNR phase of the outburst, and the energy budget of the explosion.

Affiliated with

Also associated with

No associations

Rating

Multiwavelength Observations of V1494 AQL in Outburst 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 Multiwavelength Observations of V1494 AQL in Outburst, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multiwavelength Observations of V1494 AQL in Outburst will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1488212