Published July 1, 2016 | Version v1
Journal article

eMERLIN imaging of γ-ray nova V959 Mon's surprising evolution

  • 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/10.1088/1742-6596/728/4/042002

Additional details

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