Radio Detection of SN 1985L in NGC 5033

Details Radio Detection of SN 1985L in NGC 5033 Radio Detection of SN 1985L in NGC 5033

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aj....115.1103v&link_type=abstract

The Astronomical Journal, Volume 115, Issue 3, pp. 1103-1106.

Astronomy and Astrophysics

Astronomy

6

Supernovae: Individual: Sn 1985L

Scientific paper

Observations of SN 1985L in NGC 5033 with the Very Large Array radio telescope have resulted in two detections of radio emission at 6 cm wavelength about 8 and 16 months after optical discovery. Combined with a number of upper limits and a study of possible models, these indicate that SN 1985L was probably a fairly normal Type II-L radio supernova, somewhat intermediate in radio properties between the well-studied radio supernovae SN 1979C and SN 1980K. A possible late-time optical detection, discussed in an accompanying paper by Fesen (1998), continues the observed correlation between radio and late-time optical emission.

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