The nearby Type Ia supernova (SN Ia) SN 2011fe in M101 (cz = 241 km s(-1)) provides a unique opportunity to study the early evolution of a "normal" SN Ia, its compositional structure, and its elusive ...

Matheson, T.; Joyce, R. R.; Allen, L. E.; Saha, A.; Silva, D. R.; Wood-Vasey, W. M.; Adams, J. J.; Anderson, R. E.; Beck, T. L.; Bentz, M. C.; Bershady, M. A ...

Central Bureau for Astronomical Telegrams 3606. (2013): 1. Web. Richmond, Michael W and Horace A Smith. "BVRI Photometry of SN 2011fe in M101." The Journal of the American Association of Variable Star ...

"After supernova SN 2011fe, one of the brightest ones of the last decades, this stunning 'cosmic island' offers us another huge cosmic explosion: supernova SN 2023ixf." You can't see the radiant ...

"After supernova SN 2011fe, one of the brightest ones of the last decades, this stunning 'cosmic island' offers us another huge cosmic explosion: supernova SN 2023ixf." You can't see the radiant ...

Then in 2011, the theory was overthrown. SN 2011fe, the closest Type Ia found in decades, was spotted so early in its explosion that astronomers had the chance to look for a companion star.

Then in 2011, the theory was overthrown. SN 2011fe, the closest Type Ia found in decades, was spotted so early in its explosion that astronomers had the chance to look for a companion star. None was ...

One notable example was supernova SN 2011fe, a quintessential type Ia explosion that occurred in the Pinwheel Galaxy (M101) in 2011, some 23 million light-years away. By type Ia supernova ...

Applying it to the case study of SN 2011fe gives a surprisingly good fit that can describe the light curves from explosion to a few weeks after peak brightness, as well as over a large range of fluxes ...