Artigo Acesso aberto Revisado por pares

Radio Detection of SN 1985L in NGC 5033

1998; Institute of Physics; Volume: 115; Issue: 3 Linguagem: Inglês

10.1086/300261

ISSN

1538-3881

Autores

Schuyler D. Van Dyk, Marcos J. Montes, K. W. Weiler, R. A. Sramek, N. Panagia,

Tópico(s)

Gamma-ray bursts and supernovae

Resumo

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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