Microlensing of Dusty Stellar Envelopes by a Point Mass Lens

Details Microlensing of Dusty Stellar Envelopes by a Point Mass Lens Microlensing of Dusty Stellar Envelopes by a Point Mass Lens

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jsara...2....6b&link_type=abstract

Journal of the Southeastern Association for Research in Astronomy, vol. 2, p. 6-9

Astronomy and Astrophysics

Astronomy

Techniques: Microlensing, Ism: Dust

Scientific paper

By modeling gravitational microlensing events, it is possible to study the structure of lensed sources from variable flux amplifications as the event progresses. In fact, it is quite the converse scenario of eclipse mapping. We consider microlensing events with a point mass lens and a spherically symmetric finite source that has a dusty envelope. Our goal is to model these events and understand how to map the circumstellar envelope intensity profile from a study of the variable spectral data.

Affiliated with

Also associated with

No associations

Rating

Microlensing of Dusty Stellar Envelopes by a Point Mass Lens 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 Microlensing of Dusty Stellar Envelopes by a Point Mass Lens, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Microlensing of Dusty Stellar Envelopes by a Point Mass Lens will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1067732