The $UBV$ Color Evolution of Classical Novae. IV. Time-Stretched $(U-B)_0$-$(M_B-2.5\log f_{\rm s})$ and $(V-I)_0$-$(M_I-2.5\log f_{\rm s})$ Color-Magnitude Diagrams of Novae in Outburst
Izumi Hachisu, Mariko Kato

TL;DR
This paper introduces time-stretched color-magnitude diagrams for classical novae, demonstrating their effectiveness in overlapping nova tracks and refining distance and reddening estimates, consistent with Gaia data.
Contribution
It extends previous work by proposing and validating new $(U-B)_0$-$(M_B-2.5 ext{log}f_s)$ and $(V-I)_0$-$(M_I-2.5 ext{log}f_s)$ diagrams for nova analysis.
Findings
Time-stretched color-magnitude tracks overlap for many novae.
Refined distance and reddening estimates agree with Gaia DR2.
New diagrams improve understanding of nova evolution.
Abstract
Light curves and color evolutions of two classical novae can be largely overlapped if we properly squeeze or stretch the timescale of a target nova against that of a template nova by . Then the brightness of the target nova is related to the brightness of the template nova by , where is the absolute magnitude and a function of time , and is the ratio of timescales between the target and template novae. In the previous papers of this series, we show that many novae broadly overlap in the time-stretched - color-magnitude diagram. In the present paper, we propose two other - and - diagrams, and show that their tracks overlap for 16 novae and for 52 novae, respectively. Here,…
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