Published 1983 | Version v1
Book Metadata-only

Possibilities and attempts to determine the differential rotation on F-type main-sequence stars

Creators

  • 1. Kiepenheuer-Institut fuer Sonnenphysik, Freiburg, Federal Republic of Germany

Description

A preliminary analysis of spectral lines by Fourier transformation was used to determine upper limits of differential rotation for 11 F-type stars, mainly from the main-sequence. No evidence for a much steeper differential rotation on these stars than on the Sun could be found. (Auth.)

Additional details

Publishing Information

Publisher
D. Reidel.
Imprint Place
Dordrecht (Netherlands)
ISBN
90-277-1619-6
Imprint Title
Solar and stellar magnetic fields: origins and coronal effects
Imprint Pagination
574 p.
Journal Page Range
p. 155-159.

Conference

Title
origins and coronal effects.
Acronym
International Astronomical Union symposium no. 102 on solar and stellar magnetic fields
Dates
2-6 Aug 1982.
Place
Zurich (Switzerland).

INIS

Country of Publication
Netherlands
Country of Input or Organization
Netherlands
INIS RN
15069114
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference, Numerical Data
Descriptors DEI
EMISSION SPECTRA; EXPERIMENTAL DATA; IRON IONS; MAIN SEQUENCE STARS; ROTATION; VELOCITY
Descriptors DEC
ATOMIC IONS; CHARGED PARTICLES; DATA; INFORMATION; IONS; NUMERICAL DATA; SPECTRA; STARS

Optional Information

Notes
Includes discussion. Imprint:Includes author and subject indexes.