Photometric long-term variations and superhump occurrence in the Classical Nova RR Pictoris
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/474/2/2493/22730979/stx2838.pdf
Reference58 articles.
1. Orbital period analyses for two cataclysmic variables: UZ Fornacis and V348 Puppis inside the period gap
2. Nova V5116 Sagittarii and searching for superhumps in nova remnants
3. SDSS unveils a population of intrinsically faint cataclysmic variables at the minimum orbital period
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2. TESS light curves of cataclysmic variables – II – Superhumps in old novae and novalike variables;Monthly Notices of the Royal Astronomical Society;2022-11-30
3. Life after eruption VIII: The orbital periods of novae;Monthly Notices of the Royal Astronomical Society;2020-11-10
4. On the possibilities of classical nova identifications among historical Far Eastern guest star observations;Astronomische Nachrichten;2019-08-05
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