2026RNAAS..10...51S


Query : 2026RNAAS..10...51S

2026RNAAS..10...51S - Research Notes of the AAS, 10, 51 (2026/March-0)

Modern Rate-of-decline Relations for Novae.

SHAFTER A.W.

Abstract (from CDS):

A large sample of t2 and t3 times from the recent compilation of nova properties given in B. E. Schaefer have been analyzed to determine relationships between these two parameters. Fits were performed in both directions (from ${\mathrm{log}}\,{t}_{2}$ to ${\mathrm{log}}\,{t}_{3}$ and vice-versa) to account for the asymmetry inherent in ordinary least-squares regression, which minimizes residuals only in the dependent variable. The following best-fit relations were found: ${\mathrm{log}}\,{t}_{3}=(0.877\pm 0.019){\mathrm{log}}\,{t}_{2}+(0.444\pm 0.027)$, and ${\mathrm{log}}\,{t}_{2}=(1.018\pm 0.023){\mathrm{log}}\,{t}_{3}-(0.316\pm 0.037)$, corresponding to ${t}_{3}=(2.78\pm 0.17)\,{t}_{2}^{(0.877\pm 0.019)}$ and ${t}_{2}=(0.483\pm 0.041)\,{t}_{3}^{(1.018\pm 0.023)}$, respectively. Within the uncertainties, the latter relation reduces to a simple proportionality: t2 ≃ 0.5 t3.

Abstract Copyright: © 2026. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Cataclysmic variable stars - Classical novae - Recurrent novae

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
2 V* MT Cen No* 11 44 00.8022219504 -60 33 39.546609732           ~ 21 0
3 V* V2362 Cyg CV* 21 11 32.3419758636 +44 48 03.668158208           ~ 108 0

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