1992JAVSO..21...86P


Query : 1992JAVSO..21...86P

1992JAVSO..21...86P - J. Am. Assoc. Variable star obs., 21, 86-92 (1992/December-0)

Period changes in RV Tauri stars: observations and simulations.

PERCY J.R., CSATARY A. and ZORGDRAGER I.

Abstract (from CDS):

We have determined the times and magnitudes of minimum brightness of two RV Tauri stars (SS Gem and V Vul) using data from the AAVSO and from the literature. We have used these to construct (O-C) diagrams. These are dominated by cyclic features with time scales ranging from several to several hundred pulsation periods. By constructing simulated (O-C) diagrams, we have shown that the observed (O-C) diagrams could be explained by the accumulation of random, cycle-to-cycle fluctuations in period, as in the case of most Mira stars.

Abstract Copyright: ∼

Journal keyword(s): RV Tauri stars

Simbad objects: 5

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Number of rows : 5
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* SS Gem RV* 06 08 35.1092051400 +22 37 01.988942124 10.42 9.71 8.67     G2/5I 72 0
2 V* U Mon pA* 07 30 47.4711645432 -09 46 36.757477488 8.22 7.00 5.82     G8/K0Ib/II 215 0
3 V* AC Her pA* 18 30 16.2373118976 +21 52 00.599340000 8.00 7.79 7.01     F4Ibp 359 0
4 V* R Sct RV* 18 47 28.9498974024 -05 42 18.542611800 8.30 6.67 5.20 4.14 3.37 K4/5pec 332 1
5 V* V Vul RV* 20 36 32.0211817128 +26 36 14.499788940   9.68 8.05     K0 85 0

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