The structure of a recent nova shell as observed by ALMA

High resolution ALMA observations of the recent (2.52 yr old) shell of Nova V5668 Sgr (2015) show a highly structured ionized gas distribution with small (10^15 cm) clumps. These are the smallest structures ever observed in the remnant of a stellar thermonuclear explosion. No extended contiguous emi...

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Bibliographic Details
Main Author: Diaz, Marcos (author)
Other Authors: Abraham, Zulema (author), Ribeiro, Valério A. R. M. (author), Beaklini, Pedro P. B. (author), Takeda, Larissa (author)
Format: article
Language:eng
Published: 2018
Subjects:
Stars: novae
Cataclysmic variables
Stars: white dwarfs
Radio continuum: stars
Online Access:http://hdl.handle.net/10773/24006
Country:Portugal
Oai:oai:ria.ua.pt:10773/24006

Internet

http://hdl.handle.net/10773/24006

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