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Full-Text Articles in Physical Sciences and Mathematics
Seven Years Of Sn 2014c: A Multiwavelength Synthesis Of An Extraordinary Supernova, B. P. Thomas, J. C. Wheeler, V. V. Dwarkadas, C. Stockdale, J. Vinkó, David Pooley, Y. Xu, G. Zeimann, P. Macqueen
Seven Years Of Sn 2014c: A Multiwavelength Synthesis Of An Extraordinary Supernova, B. P. Thomas, J. C. Wheeler, V. V. Dwarkadas, C. Stockdale, J. Vinkó, David Pooley, Y. Xu, G. Zeimann, P. Macqueen
Physics and Astronomy Faculty Research
SN 2014C was originally classified as a Type Ib supernova, but at phase ϕ = 127 days, post-explosion strong Hα emission was observed. SN 2014C has since been observed in radio, infrared, optical and X-ray bands. Here we present new optical spectroscopic and photometric data spanning ϕ = 947–2494 days post-explosion. We address the evolution of the broadened Hα emission line, as well as broad [O iii] emission and other lines. We also conduct a parallel analysis of all publicly available multiwavelength data. From our spectra, we find a nearly constant Hα FWHM velocity width of ∼2000 …
X-Ray Swift Observations Of Sn 2018cow, L E. Rivera Sandoval, T J. Maccarone, A Corsi, P J. Brown, David Pooley, J C. Wheeler
X-Ray Swift Observations Of Sn 2018cow, L E. Rivera Sandoval, T J. Maccarone, A Corsi, P J. Brown, David Pooley, J C. Wheeler
Physics and Astronomy Faculty Research
Supernova (SN) 2018cow is an optical transient detected in the galaxy CGCG 137–068. It has been classified as a SN due to various characteristics in its optical spectra. The transient is also a bright X-ray source. We present results of the analysis of ∼ 62 ks of X-ray observations taken with the Neil Gehrels Swift Observatory over 27 days. We found a variable behavior in the 0 . 3 − 10 keV X-ray light curve of SN 2018cow, with variability timescales of days. The observed X-ray variability could be due to the interaction between the SN ejecta and a non-uniform …