A high angular-resolution search for the progenitor of the type Ic Supernova 2004gt

Details A high angular-resolution search for the progenitor of the type Ic Supernova 2004gt A high angular-resolution search for the progenitor of the type Ic Supernova 2004gt

2005-06-21

arxiv.org/abs/astro-ph/0506472v3

Astrophys.J.630:L29-L32,2005

Astronomy and Astrophysics

Astrophysics

ApJ Letters, in press. Revised version to match accepted version, minor changes following referee report. Version with full re

Scientific paper

10.1086/491622

We report the results of a high-spatial-resoltion search for the progenitor of type Ic supernova SN 2004gt, using the newly commissioned Keck laser-guide star adaptive optics system (LGSAO) along with archival Hubble Space Telescope data. This is the deepest search yet performed for the progenitor of any type Ib/c event in a wide wavelength range stretching from the far UV to the near IR. We determine that the progenitor of SN 2004gt was most likely less luminous than M_V=-5.5 and M_B=-6.5 magnitudes. The massive stars exploding as hydrogen-deficient core-collapse supernovae (SNe) should have lost their outer hydrogen envelopes prior to their explosion, either through winds -- such stars are identified within our Galaxy as Wolf-Rayet (W-R) stars -- or to a binary companion. The luminosity limits we set rule out more than half of the known galactic W-R stars as possible progenitors of this event. In particular, they imply that a W-R progenitor should have been among the more-evolved (highly stripped, less luminous) of these stars, a concrete constraint on its evolutionary state just prior to core collapse. The possibility of a less luminous, lower-mass binary progenitor cannot be constrained. This study demonstrates the power of LGS observations in furthering our understanding of core collapse, and the physics powering supernovae, GRBs and XRFs.

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