No pre-maximum halt in classical nova V5589 Sgr observed with STEREO HI-1B
Author:
Funder
National Aeronautics and Space Administration (NASA)
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/470/4/4061/18772951/stx1552.pdf
Reference27 articles.
1. Determination of the Photometric Calibration and Large-Scale Flatfield of the STEREO Heliospheric Imagers: I. HI-1
2. Calibrating the Pointing and Optical Parameters of the STEREO Heliospheric Imagers
3. ON THE PROGENITORS OF GALACTIC NOVAE
4. Temporal resolution of a pre-maximum halt in a classical nova: V5589 Sgr observed with STEREO HI-1B
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1. New Insights into Classical Novae;Annual Review of Astronomy and Astrophysics;2021-09-08
2. The UBV Color Evolution of Classical Novae. IV. Time-stretched (U − B)0–(M B − 2.5 log f s) and (V − I)0–(M I − 2.5 log f s) Color–Magnitude Diagrams of Novae in Outbursts;The Astrophysical Journal Supplement Series;2021-03-01
3. A Light-curve Analysis of 32 Recent Galactic Novae: Distances and White Dwarf Masses;The Astrophysical Journal Supplement Series;2019-05-31
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