2003IBVS.5483....1T


Query : 2003IBVS.5483....1T

2003IBVS.5483....1T - IAU Inform. Bull. Var. Stars, 5483, 1 (2003/December-0)

A revised period for the mira variable AW Aurigae.

TEMPLETON M.R.

Abstract (from CDS):

AW Aurigae is listed in the GCVS as a Mira variable with a period of 695 days, one of the longest among the Miras. However, the period was considered preliminary when first determined by Kurochkin (1951) and the original ephemeris of Max = JD 2429200 + 695 X E produced very large (O-C) residuals. Analysis of visual and V-band data from the AAVSO International Database and photometry from the Harvard College Observatory plate collection yields a best-fitting period of 449.3 ± 0.7 days.

Abstract Copyright: ∼

Journal keyword(s): Miras: time-series

Simbad objects: 2

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Number of rows : 2
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 V* AW Aur Mi* 05 40 00.6849318168 +28 42 48.627475920       10.19   M8 37 0
2 V* Z Tau S* 05 52 24.8532067728 +15 47 43.764061776     10.11 13.87   S7.51e 59 0

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