Structures and Expansions of SN 1993J and SN 2004et

Details Structures and Expansions of SN 1993J and SN 2004et Structures and Expansions of SN 1993J and SN 2004et

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lnea....2..215m&link_type=abstract

Lecture Notes and Essays in Astrophysics, vol. 2, p. 215-226.

Astronomy and Astrophysics

Astrophysics

Supernovae, Radio Emission, Vlbi

Scientific paper

Radio emission has been detected from a small subset of supernovae. For those radio supernovae that are strong radio emitters and are not too distant (≤20 Mpc) VLBI observations have been performed and, in some cases, high angular resolution images obtained. Thanks to VLBI observations, source structures and expansion decelerations have been determined. Together with multi-wavelength light curves and optical spectra, these observations have helped characterize the supernova ejecta and the circumstellar medium density profiles. We report on VLBI observations of SN1993J and SN2004et. In the case of supernova SN~1993J, the details of the expansion have been determined with astonishing detail. In the case of supernova SN~2004et, the last radio supernova imaged with VLBI, some considerations about the physical conditions in which this supernova evolves are made.

Affiliated with

Also associated with

No associations

Rating

Structures and Expansions of SN 1993J and SN 2004et 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 Structures and Expansions of SN 1993J and SN 2004et, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structures and Expansions of SN 1993J and SN 2004et will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1548215