Shock shaping? Nebular spectroscopy of nova V906 Carinae

Author:

Harvey É J1ORCID,Aydi E2,Izzo L3ORCID,Morisset C4,Darnley M J1ORCID,Fitzgerald K5ORCID,Molaro P6ORCID,Murphy-Glaysher F1,Redman M P7,Shrestha M18

Affiliation:

1. Astrophysics Research Institute, Liverpool John Moores University , IC2 Liverpool Science Park, Liverpool L3 5RF , UK

2. Center for Data Intensive and Time Domain Astronomy, Department of Physics and Astronomy, Michigan State University , East Lansing, MI 48824 , USA

3. DARK, Niels Bohr Institute, University of Copenhagen , Jagtvej 128, DK-2200 Copenhagen , Denmark

4. Universidad Nacional Autónoma de México , Instituto de Astronomía, AP 106, Ensenada 22800, BC , México

5. Technological University of the Shannon , Athlone Campus, Co. Westmeath, N37HD68 Athlone , Ireland

6. Osservatorio Astronomico di Trieste , Vuz GB Trepolo 11, I-34131, Trieste , Italy

7. National University of Ireland, Galway to University of Galway , H91 TK33 Galway , Ireland

8. Steward Observatory, University of Arizona , 933 North Cherry Avenue, Tucson, AZ 85721-0065 , USA

Abstract

ABSTRACT V906 Carinae was one of the best observed novae of recent times. It was a prolific dust producer and harboured shocks in the early evolving ejecta outflow. Here, we take a close look at the consequences of these early interactions through study of high-resolution Ultraviolet and Visual Echelle spectrograph spectroscopy of the nebular stage and extrapolate backwards to investigate how the final structure may have formed. A study of ejecta geometry and shaping history of the structure of the shell is undertaken following a spectral line $\rm {\small SHAPE}$ model fit. A search for spectral tracers of shocks in the nova ejecta is undertaken and an analysis of the ionized environment. Temperature, density, and abundance analyses of the evolving nova shell are presented.

Funder

STFC

NASA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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