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The Astrophysical Journal
Article . 1998 . Peer-reviewed
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https://dx.doi.org/10.1086/306...
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The Spectroscopic Differences between Disk and Thick‐Disk/Bulge Novae

descriptionPublicationkeyboard_double_arrow_right Article 20 Oct 1998 English Publisher:American Astronomical SocietyJournal:The Astrophysical Journal, volume 506, pages 818-823 (issn: 0004-637X, eissn: 1538-4357, Copyright policy )
Authors: Massimo Della Valle; Mario Livio;

doi: 10.1086/306275

The Spectroscopic Differences between Disk and Thick‐Disk/Bulge Novae

Abstract

We examine a sample of novae with distances that have been mostly determined by nebular parallaxes and determine their spectral classes according to the classification of Williams. We show that novae that have been classified as He/N tend to concentrate close to the Galactic plane and are fast and bright, while Fe II novae are slow and faint and are distributed more homogeneously up to heights of ~1000 pc above the Galactic plane. We identify a quantitative characterization of the prototypical "fast" and "slow" novae.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
74
Top 10%
Top 10%
Top 10%
gold
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