Nonlinear beat Cepheid models

被引:39
作者
Kolláth, Z
Beaulieu, JP
Buchler, JR
Yecko, P
机构
[1] Konkoly Observ Budapest, H-1525 Budapest XII, Hungary
[2] Kapteyn Astron Inst, NL-9700 AV Groningen, Netherlands
[3] Univ Florida, Dept Phys, Gainesville, FL 32611 USA
基金
美国国家科学基金会; 匈牙利科学研究基金会;
关键词
Cepheids; convection; hydrodynamics; Magellanic Clouds; stars : oscillations; turbulence;
D O I
10.1086/311484
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The numerical hydrodynamic modeling of beat Cepheid behavior has been a long-standing quest in which purely radiative models have failed miserably. We find that beat pulsations occur naturally when turbulent convection is accounted for in our hydrodynamics codes. The development of a relaxation code and of a Floquet stability analysis greatly facilitates the search for and analysis of beat Cepheid models. The conditions for the occurrence of beat behavior can be understood easily and at a fundamental level with the help of amplitude equations. Here a discriminant D arises whose sign decides whether single-mode or double-mode pulsations can occur in a model, and this D depends only on the values of the nonlinear coupling coefficients between the fundamental and the first overtone modes. For radiative models D is always found to be negative, but with sufficiently strong turbulent convection its sign reverses.
引用
收藏
页码:L55 / L58
页数:4
相关论文
共 12 条
[1]   LOW-TEMPERATURE ROSSELAND OPACITIES [J].
ALEXANDER, DR ;
FERGUSON, JW .
ASTROPHYSICAL JOURNAL, 1994, 437 (02) :879-891
[2]   PULSATION AND STABILITY OF RR LYRAE STARS .1. INSTABILITY STRIP [J].
BONO, G ;
STELLINGWERF, RF .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1994, 93 (01) :233-269
[3]  
Buchler JR, 1998, ASTR SOC P, V135, P220
[4]   ON THE MODAL SELECTION OF RADIAL STELLAR PULSATORS [J].
BUCHLER, JR ;
KOVACS, G .
ASTROPHYSICAL JOURNAL, 1986, 308 (02) :661-668
[5]   PERIODIC STELLAR PULSATIONS - STABILITY ANALYSIS AND AMPLITUDE EQUATIONS [J].
BUCHLER, JR ;
MOSKALIK, P ;
KOVACS, G .
ASTROPHYSICAL JOURNAL, 1991, 380 (01) :185-199
[6]  
GEHMEYR M, 1992, ASTRON ASTROPHYS, V253, P92
[7]   Updated OPAL opacities [J].
Iglesias, CA ;
Rogers, FJ .
ASTROPHYSICAL JOURNAL, 1996, 464 (02) :943-953
[8]  
KOVACS G, 1987, APJ, V324, P1026
[9]  
KUHFUSS R, 1986, ASTRON ASTROPHYS, V160, P116
[10]   CONVECTION IN PULSATING STARS .1. NON-LINEAR HYDRODYNAMICS [J].
STELLINGWERF, RF .
ASTROPHYSICAL JOURNAL, 1982, 262 (01) :330-338