The peculiar mass-loss history of SN 2014C as revealed through AMI radio observations
We present a radio light curve of supernova (SN) 2014C taken with the Arcminute Microkelvin Imager (AMI) Large Array at 15.7 GHz. Optical observations presented by Milisavljevic et al. demonstrated that SN 2014C metamorphosed from a stripped-envelope Type Ib SN into a strongly interacting Type IIn S...
المؤلفون الرئيسيون: | Anderson, G, Horesh, A, Mooley, K, Rushton, A, Fender, R, Staley, T, Argo, M, Beswick, R, Hancock, P, Pérez-Torres, M, Perrott, Y, Plotkin, R, Pretorius, M, Rumsey, C, Titterington, D |
---|---|
التنسيق: | Journal article |
منشور في: |
Oxford University Press
2016
|
مواد مشابهة
-
On the use of variability time-scales as an early classifier of radio transients and variables
حسب: Pietka, M, وآخرون
منشور في: (2017) -
Rapid radio flaring during an anomalous outburst of SS Cyg
حسب: Mooley, K, وآخرون
منشور في: (2017) -
A detailed radio study of the energetic, nearby, and puzzling GRB 171010A
حسب: Bright, JS, وآخرون
منشور في: (2019) -
Long-term radio and X-ray evolution of the tidal disruption event ASASSN-14li
حسب: Bright, JS, وآخرون
منشور في: (2018) -
The Arcminute Microkelvin Imager catalogue of gamma-ray burst afterglows at 15.7 GHz
حسب: Anderson, G, وآخرون
منشور في: (2017)