2003IBVS.5367....1T


Query : 2003IBVS.5367....1T

2003IBVS.5367....1T - IAU Inform. Bull. Var. Stars, 5367, 1 (2003/January-0)

LX Cygni: a mira variable with a drastic period increase.

TEMPLETON M.R., MATTEI J.A. and PRICE A.

Abstract (from CDS):

The Mira variable LX Cygni has been undergoing significant period increase over the entire span of the AAVSO archives (JD 2439800 - 2453000) from 460 d to 580 d. The period change appears to be continuous rather than a discrete jump, which argues against a mode switch as the cause. LX Cygni may be in the midst of a thermal pulse, and more observations are encouraged.

Abstract Copyright: ∼

Journal keyword(s): Miras, photometry, Miras, asteroseismology

Simbad objects: 3

goto View the references in ADS

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 V* TY Cas Mi* 00 36 59.3979390720 +63 08 01.809743388     13.20 11.57   M8 53 0
2 V* T UMi Mi* 13 34 41.0716584144 +73 25 53.083879752   12.54 11.46     M6e 104 0
3 V* LX Cyg C* 21 55 57.0262652688 +48 20 52.522680876   13.22 10.49 10.52   C 44 1

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