Nova Eruptions with Infrared Interferometric Observations

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

Infrared interferometric observations have a great deal of potential to unravel the nature of the nova eruptions. We suggest that techniques, already in place, to derive the ejection details at optical wavelengths be used with infrared interferometric observations to derive parameters such as the ejected mass in a nova eruption. This is achievable based on modelling the initial phase of the eruption when the infrared light is dominated by the free-free thermal process.

Original languageEnglish
Title of host publicationThe Physics of Evolved Stars
Subtitle of host publicationA Conference Dedicated to the Memory of Olivier Chesneau
EditorsF. Millour, T. Lanz, E. Lagadec
PublisherEDP Sciences
Pages137-141
Number of pages5
ISBN (Electronic)9782759819072
DOIs
Publication statusPublished - Dec 1 2015
EventPhysics of Evolved Stars Conference 2015 - Nice, France
Duration: Jun 8 2015Jun 12 2015

Publication series

NameEAS Publications Series
Volume71-72
ISSN (Print)1633-4760
ISSN (Electronic)1638-1963

Other

OtherPhysics of Evolved Stars Conference 2015
CountryFrance
CityNice
Period6/8/156/12/15

All Science Journal Classification (ASJC) codes

  • Engineering(all)

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  • Cite this

    Ribeiro, V. A. R. M. (2015). Nova Eruptions with Infrared Interferometric Observations. In F. Millour, T. Lanz, & E. Lagadec (Eds.), The Physics of Evolved Stars: A Conference Dedicated to the Memory of Olivier Chesneau (pp. 137-141). (EAS Publications Series; Vol. 71-72). EDP Sciences. https://doi.org/10.1051/eas/1571029