Search: WFRF:(Roettenbacher Rachael M.)
> (2017) >
Surface magnetism o...
Surface magnetism of cool stars
-
- Kochukhov, Oleg (author)
- Uppsala universitet,Observationell astrofysik
-
- Petit, P. (author)
- Univ Toulouse, UPS OMP, IRAP, Toulouse, France.;CNRS, Inst Rech Astrophys & Planetol, Toulouse, France.
-
- Strassmeier, K. G. (author)
- Leibniz Inst Astrophys Potsdam AIP, Potsdam, Germany.
-
show more...
-
- Carroll, T. A. (author)
- Leibniz Inst Astrophys Potsdam AIP, Potsdam, Germany.
-
- Fares, R. (author)
- Osserv Astrofis Catania, INAF, Catania, Italy.
-
- Folsom, C. P. (author)
- Univ Toulouse, UPS OMP, IRAP, Toulouse, France.;CNRS, Inst Rech Astrophys & Planetol, Toulouse, France.
-
- Jeffers, S. V. (author)
- Georg August Univ Gottingen, Inst Astrophys, Gottingen, Germany.
-
- Korhonen, H. (author)
- Univ Copenhagen, Niels Bohr Inst, Copenhagen, Denmark.
-
- Monnier, J. D. (author)
- Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA.
-
- Morin, J. (author)
- Univ Montpellier, CNRS, LUPM, Montpellier, France.
-
- Rosén, Lisa (author)
- Uppsala universitet,Observationell astrofysik
-
- Roettenbacher, Rachael M. (author)
- Stockholms universitet,Institutionen för astronomi,University of Michigan, USA
-
- Shulyak, D. (author)
- Georg August Univ Gottingen, Inst Astrophys, Gottingen, Germany.
-
show less...
-
(creator_code:org_t)
- 2017-03-17
- 2017
- English.
-
In: Astronomical Notes - Astronomische Nachrichten. - : WILEY-V C H VERLAG GMBH. - 0004-6337 .- 1521-3994. ; 338:4, s. 428-441
- Related links:
-
https://onlinelibrar...
-
show more...
-
https://urn.kb.se/re...
-
https://doi.org/10.1...
-
https://urn.kb.se/re...
-
show less...
Abstract
Subject headings
Close
- Magnetic fields are essential ingredients of many physical processes in the interiors and envelopes of cool stars. Yet their direct detection and characterization is notoriously difficult, requiring high-quality observations and advanced analysis techniques. Significant progress has been recently achieved by several types of direct magnetic field studies on the surfaces of cool, active stars. In particular, complementary techniques of field topology mapping with polarization data and total magnetic flux measurements from intensity spectra have been systematically applied to different classes of active stars, leading to interesting and occasionally controversial results. In this paper, we summarize the current status of direct magnetic field studies of cool stars and investigations of surface inhomogeneities caused by the field, based on the material presented at the Cool Stars 19 splinter session.
Subject headings
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Keyword
- stars: activity
- stars: late-type
- stars: low-mass
- stars: magnetic field
- starspots
Publication and Content Type
- ref (subject category)
- art (subject category)
Find in a library
To the university's database
- By the author/editor
-
Kochukhov, Oleg
-
Petit, P.
-
Strassmeier, K. ...
-
Carroll, T. A.
-
Fares, R.
-
Folsom, C. P.
-
show more...
-
Jeffers, S. V.
-
Korhonen, H.
-
Monnier, J. D.
-
Morin, J.
-
Rosén, Lisa
-
Roettenbacher, R ...
-
Shulyak, D.
-
show less...
- About the subject
-
- NATURAL SCIENCES
-
NATURAL SCIENCES
-
and Physical Science ...
-
and Astronomy Astrop ...
- Articles in the publication
-
Astronomical Not ...
- By the university
-
Uppsala University
-
Stockholm University