Published 1979 | Version v1
Report Restricted

Time-scale for turn-off of a nova after the outburst

Creators

Description

Theoretical and observational evidence is reviewed for the remnant from a nova outburst. Its evolution to burnout is described. Finally, the various physical mechanisms which can lead to an extended period of mass loss are discussed. 19 references

Availability note (English)

MF available from INIS under the Report Number; Available from NTIS., PC A02/MF A01.

Files

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Additional details

Additional titles

Augmented title (English)
Mass loss extended period, mechanisms

Publishing Information

Imprint Pagination
7 p.
Report number
LA-UR--79-2044

Conference

Title
IAU colloquium on the structure of white dwarfs and variable degenerates.
Dates
30 Jul - 3 Aug 1979.
Place
Rochester, NY, USA.

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
11503936
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
KINETICS; MASS TRANSFER; NOVAE; STAR EVOLUTION; TIME DEPENDENCE
Descriptors DEC
ERUPTIVE VARIABLE STARS; STARS; VARIABLE STARS

Optional Information

Secondary number(s)
CONF-790755--2.