|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
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
To bookmark this query, right click on this link: simbad:2003IBVS.5367....1T and select 'bookmark this link' or equivalent in the popup menu