Activity cycle periods in late-type stars

N. I. Kleeorin; A. A. Ruzmaikin; D. D. Sokoloff

doi:10.1007/BF00661164

Activity cycle periods in late-type stars

N. I. Kleeorin, A. A. Ruzmaikin, D. D. Sokoloff

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

10 Scopus citations

Abstract

Period of magnetic activity versus the stellar angular velocity for stars of given spectral type having extended convective shells is estimated within the framework of mean field dynamo theory. The dependence appears to be not monotonous, and can be checked by observations.

Original language	English
Pages (from-to)	131-136
Number of pages	6
Journal	Astrophysics and Space Science
Volume	95
Issue number	1
DOIs	https://doi.org/10.1007/BF00661164
State	Published - 1 Jan 1983
Externally published	Yes

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1007/BF00661164

Cite this

@article{e3f17e72afcf49cc919d964892d90252,

title = "Activity cycle periods in late-type stars",

abstract = "Period of magnetic activity versus the stellar angular velocity for stars of given spectral type having extended convective shells is estimated within the framework of mean field dynamo theory. The dependence appears to be not monotonous, and can be checked by observations.",

author = "Kleeorin, {N. I.} and Ruzmaikin, {A. A.} and Sokoloff, {D. D.}",

year = "1983",

month = jan,

day = "1",

doi = "10.1007/BF00661164",

language = "English",

volume = "95",

pages = "131--136",

journal = "Astrophysics and Space Science",

issn = "0004-640X",

publisher = "Springer Netherlands",

number = "1",

}

TY - JOUR

T1 - Activity cycle periods in late-type stars

AU - Kleeorin, N. I.

AU - Ruzmaikin, A. A.

AU - Sokoloff, D. D.

PY - 1983/1/1

Y1 - 1983/1/1

N2 - Period of magnetic activity versus the stellar angular velocity for stars of given spectral type having extended convective shells is estimated within the framework of mean field dynamo theory. The dependence appears to be not monotonous, and can be checked by observations.

AB - Period of magnetic activity versus the stellar angular velocity for stars of given spectral type having extended convective shells is estimated within the framework of mean field dynamo theory. The dependence appears to be not monotonous, and can be checked by observations.

UR - http://www.scopus.com/inward/record.url?scp=0039093578&partnerID=8YFLogxK

U2 - 10.1007/BF00661164

DO - 10.1007/BF00661164

M3 - Article

AN - SCOPUS:0039093578

SN - 0004-640X

VL - 95

SP - 131

EP - 136

JO - Astrophysics and Space Science

JF - Astrophysics and Space Science

IS - 1

ER -

Activity cycle periods in late-type stars

Abstract

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this