Interferometric observations of explosive variables: V838 mon, nova Aql 2005 & RS Oph

Benjamin F. Lane, Alon Retter, Joshua A Eisner, Robert R. Thompson, Matthew W. Muterspaugh

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

1 Scopus citations

Abstract

During the last two years we have used the Palomar Testbed Interferometer to observe several explosive variable stars, including V838 Monocerotis, V1663 Aquilae and recently RS Ophiuchi. We observed V838 Monocerotis approximately 34 months after its eruption, and were able to resolve the ejecta. Observations of V1663 Aql were obtained starting 9 days after peak brightness and continued for 10 days. We were able to resolve the milliarcsecond-scale emission and follow the expansion of the nova photosphere. When combined with radial-velocity information, these observations can be used to infer the distance to the nova. Finally we have resolved the recurrent nova RS Oph and can draw some preliminary conclusions regarding the emission morphology.

Original languageEnglish (US)
Title of host publicationProceedings of SPIE - The International Society for Optical Engineering
Volume6268 I
DOIs
Publication statusPublished - 2006
Externally publishedYes
EventAdvances in Stellar Interferometry - Orlando, FL, United States
Duration: May 25 2006May 30 2006

Other

OtherAdvances in Stellar Interferometry
CountryUnited States
CityOrlando, FL
Period5/25/065/30/06

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Keywords

  • Distances
  • Novae
  • Techniques - interferometric

ASJC Scopus subject areas

  • Electrical and Electronic Engineering
  • Condensed Matter Physics

Cite this

Lane, B. F., Retter, A., Eisner, J. A., Thompson, R. R., & Muterspaugh, M. W. (2006). Interferometric observations of explosive variables: V838 mon, nova Aql 2005 & RS Oph. In Proceedings of SPIE - The International Society for Optical Engineering (Vol. 6268 I). [62681K] https://doi.org/10.1117/12.674431