Possible Recovery of SN 1961V In Hubble Space Telescope Archival Images

摘要

SN 1961V in NGC 1058 was originally classified by Fritz Zwicky as a ``TypeV'' supernova. However, it has been argued that SN 1961V was not a genuinesupernova, but instead the superoutburst of an eta Carinae-like luminous bluevariable star. In particular, Filippenko et al. (1995, AJ, 110, 2261) usedpre-refurbishment HST WFPC images and the known radio position of SN 1961V toconclude that the star survived the eruption and is likely coincident with a V~ 25.6 mag, V-I ~ 1.9 mag object. Recently, Stockdale et al. (2001, AJ, 122,283) recovered the fading SN 1961V at radio wavelengths and argue that itsbehavior is similar that of some Type II supernovae. We have analyzedpost-refurbishment archival HST WFPC2 data and find that the new radio positionis still consistent with the Filippenko et al. object, which has not changed inbrightness or color, but is also consistent with an adjacent, fainter (I ~ 24.3mag) and very red (V-I > 1.0 mag) object. We suggest that this fainter objectcould be the survivor of SN 1961V. Forthcoming HST observations may settle thisissue.