Published July 1, 2016
| Version v1
Journal article
eMERLIN imaging of γ-ray nova V959 Mon's surprising evolution
Creators
- 1. Jodrell Bank Centre for Astrophysics, Alan Turing Building, University of Manchester, Oxford Road, Manchester M13 9PL (United Kingdom)
Description
High resolution radio images of γ-ray nova V959 Mon using e-MERLIN are presented here, at epochs in September 2012, November 2012, February 2013, October 2013 and February 2014. A light curve at C-Band frequency has been produced which is in good agreement with contemporaneous VLA observations. While early e-MERLIN observations of V959 Mon appear to show an east-west elongation in the ejecta morphology, subsequent observations show that the ejecta are now elongated in the north-south direction. Our high-resolution observations of the structure of V959 Mon can assist us in further understanding the mechanisms of mass ejection from novae. (paper)
Availability note (English)
Available from http://dx.doi.org/10.1088/1742-6596/728/4/042002Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Physics. Conference Series (Online)
- Journal Volume
- 728
- Journal Issue
- 4
- Journal Page Range
- [4 p.]
- ISSN
- 1742-6596
Conference
- Title
- Physics and chemistry of the late stages of stellar evolution
- Acronym
- 11. Pacific Rim conference on stellar astrophysics
- Dates
- 14-17 Dec 2015
- Place
- Hong Kong (China)
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 48100359
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; COSMIC GAMMA SOURCES; COSMIC RADIO SOURCES; GAMMA RADIATION; IMAGES; MASS; MORPHOLOGY; NOVAE; RESOLUTION; VISIBLE RADIATION
- Descriptors DEC
- BINARY STARS; COSMIC RAY SOURCES; ELECTROMAGNETIC RADIATION; ERUPTIVE VARIABLE STARS; IONIZING RADIATIONS; PHYSICS; RADIATIONS; STARS; VARIABLE STARS