On the pulsation mode of Mira variables: Nonlinear calculations compared with radii observations

A. Ya'ari; Y. Tuchman

doi:10.1086/311932

On the pulsation mode of Mira variables: Nonlinear calculations compared with radii observations

A. Ya'ari^*, Y. Tuchman

^*Corresponding author for this work

Racah Institute of Physics

Research output: Contribution to journal › Article › peer-review

15 Scopus citations

Abstract

Observed radii of Mira variables are compared with theoretical nonlinear calculations. In contrast with previous works, the observed data is found to be compatible with the fundamental nonlinear mode of pulsation.

Original language	English
Pages (from-to)	L35-L37
Journal	Astrophysical Journal
Volume	514
Issue number	1 PART 2
DOIs	https://doi.org/10.1086/311932
State	Published - 20 Mar 1999

Keywords

Stars: fundamental parameters
Stars: late-type
Stars: oscillations

Access to Document

10.1086/311932

Cite this

@article{d324e571e8364732a9efea1a8585d4bf,

title = "On the pulsation mode of Mira variables: Nonlinear calculations compared with radii observations",

abstract = "Observed radii of Mira variables are compared with theoretical nonlinear calculations. In contrast with previous works, the observed data is found to be compatible with the fundamental nonlinear mode of pulsation.",

keywords = "Stars: fundamental parameters, Stars: late-type, Stars: oscillations",

author = "A. Ya'ari and Y. Tuchman",

year = "1999",

month = mar,

day = "20",

doi = "10.1086/311932",

language = "אנגלית",

volume = "514",

pages = "L35--L37",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing Ltd.",

number = "1 PART 2",

}

TY - JOUR

T1 - On the pulsation mode of Mira variables

T2 - Nonlinear calculations compared with radii observations

AU - Ya'ari, A.

AU - Tuchman, Y.

PY - 1999/3/20

Y1 - 1999/3/20

N2 - Observed radii of Mira variables are compared with theoretical nonlinear calculations. In contrast with previous works, the observed data is found to be compatible with the fundamental nonlinear mode of pulsation.

AB - Observed radii of Mira variables are compared with theoretical nonlinear calculations. In contrast with previous works, the observed data is found to be compatible with the fundamental nonlinear mode of pulsation.

KW - Stars: fundamental parameters

KW - Stars: late-type

KW - Stars: oscillations

UR - http://www.scopus.com/inward/record.url?scp=0033586041&partnerID=8YFLogxK

U2 - 10.1086/311932

DO - 10.1086/311932

M3 - ???researchoutput.researchoutputtypes.contributiontojournal.article???

AN - SCOPUS:0033586041

SN - 0004-637X

VL - 514

SP - L35-L37

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1 PART 2

ER -

On the pulsation mode of Mira variables: Nonlinear calculations compared with radii observations

Abstract

Keywords

Access to Document

Other files and links

Fingerprint

Cite this