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Constraints on the Binary Companion to the SN Ic 1994I Progenitor
Schuyler D. Van Dyk, Selma E. de Mink, Emmanouil Zapartas
Core-collapse supernovae (SNe), marking the deaths of massive stars, are among the most powerful explosions in the Universe, responsible, e.g., for a predominant synthesis of chemi…
An Excess of Mid-Infrared Emission from the Type Iax SN 2014dt
Ori D. Fox, Joel Johansson, Mansi Kasliwal +12
Supernovae Type Iax (SNe Iax) are less energetic and less luminous than typical thermonuclear explosions. A suggested explanation for the observed characteristics of this subclass…
What Powers the 3000-Day Light Curve of SN 2006gy?
Ori D. Fox, Nathan Smith, S. Mark Ammons +11
SN 2006gy was the most luminous SN ever observed at the time of its discovery and the first of the newly defined class of superluminous supernovae (SLSNe). The extraordinary energe…
Finding Wolf-Rayet Stars in the Milky Way: Inputs to Star Formation and Stellar Evolution
A. P. Marston, J. Mauerhan, P. Morris +1
The total population of Wolf-Rayet (WR) stars in the Galaxy is predicted by models to be as many as 6000 stars, and yet the number of catalogued WR stars as a result of optic…