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The Astrophysical Journal Letters, ISSN 2041-8205, 01/2012, Volume 744, Issue 2, p. L17
2012ApJ...744L..17B While a white dwarf is, from a theoretical perspective, the most plausible primary star in Type Ia supernova (SN Ia), many other candidates... 
supernovae: general | supernovae: individual (2011fe, white dwarfs) | LUMINOSITY | X RADIATION | NEUTRON STARS | MAIN SEQUENCE STARS | CARBON BURNING | SENSITIVITY | NICKEL 56 | SUPERNOVAE | DENSITY | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | ASTROPHYSICS | HELIUM BURNING | MASS | WHITE DWARF STARS | ROCHE EQUIPOTENTIALS | DETECTION | HYDROGEN BURNING | BRIGHTNESS
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 01/2010, Volume 708, Issue 2, pp. 1025 - 1031
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The Astrophysical Journal Letters, ISSN 2041-8205, 04/2011, Volume 730, Issue 2, p. L34
Journal Article
Astrophysical Journal, ISSN 0004-637X, 2014, Volume 783, Issue 2, pp. 69 - 8
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