Stellar rotation

Results: 66



#Item
51K2 Proposal on behalf of KASC WG3 Asteroseismology of Beta Cephei stars Prepared by Victoria Antoci, Peter De Cat, Luis Balona and Gerald Handler Even nowadays, the interior structure of main sequence stars and their te

K2 Proposal on behalf of KASC WG3 Asteroseismology of Beta Cephei stars Prepared by Victoria Antoci, Peter De Cat, Luis Balona and Gerald Handler Even nowadays, the interior structure of main sequence stars and their te

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Source URL: keplerscience.arc.nasa.gov

Language: English - Date: 2014-05-14 17:08:39
52SOLAR PHYSICS AND TERRESTRIAL EFFECTS   Activity 8

SOLAR PHYSICS AND TERRESTRIAL EFFECTS   Activity 8

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Source URL: www.swpc.noaa.gov

Language: English - Date: 1998-04-20 15:00:25
53Rotation of M dwarfs: spindown, activity, and gyrochronology Aleks Scholz (St Andrews), Beate Stelzer (Palermo), Sean Matt (Exeter) We propose to use K2 to measure rotation periods in a sample of nearby M dwarfs. Stellar

Rotation of M dwarfs: spindown, activity, and gyrochronology Aleks Scholz (St Andrews), Beate Stelzer (Palermo), Sean Matt (Exeter) We propose to use K2 to measure rotation periods in a sample of nearby M dwarfs. Stellar

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Source URL: keplerscience.arc.nasa.gov

Language: English - Date: 2014-05-14 17:08:39
54The fast spin-rotation of a young extra-solar planet Ignas A. G. Snellen1, Bernhard R. Brandl1, Remco J. de Kok1,2, Matteo Brogi1, Jayne Birkby1, and Henriette Schwarz1 1 Leiden Observatory, Leiden University, Postbus 9

The fast spin-rotation of a young extra-solar planet Ignas A. G. Snellen1, Bernhard R. Brandl1, Remco J. de Kok1,2, Matteo Brogi1, Jayne Birkby1, and Henriette Schwarz1 1 Leiden Observatory, Leiden University, Postbus 9

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Source URL: www.eso.org

Language: English - Date: 2014-03-21 06:11:02
55

PDF Document

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Source URL: www.modern-medical-science.site88.net

Language: English - Date: 2013-02-01 20:01:31
56Chapter 5 Properties of Disk Galaxies Disk galaxies are typically composite systems, built from several stellar populations. Besides a thin, rotating disk, such galaxies often include thicker disks or spheroids.

Chapter 5 Properties of Disk Galaxies Disk galaxies are typically composite systems, built from several stellar populations. Besides a thin, rotating disk, such galaxies often include thicker disks or spheroids.

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Source URL: www.ifa.hawaii.edu

Language: English - Date: 2009-02-12 21:15:43
57ApJ in press Preprint typeset using LATEX style emulateapj v[removed]EVIDENCE FOR THE TIDAL DESTRUCTION OF HOT JUPITERS BY SUBGIANT STARS Kevin C. Schlaufman1 and Joshua N. Winn2

ApJ in press Preprint typeset using LATEX style emulateapj v[removed]EVIDENCE FOR THE TIDAL DESTRUCTION OF HOT JUPITERS BY SUBGIANT STARS Kevin C. Schlaufman1 and Joshua N. Winn2

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Source URL: arxiv.org

Language: English - Date: 2013-06-04 20:14:32
58The Mass Distribution and Rotation Curve in the Galaxy Yoshiaki Sofue

The Mass Distribution and Rotation Curve in the Galaxy Yoshiaki Sofue

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Source URL: www.ioa.s.u-tokyo.ac.jp

Language: English - Date: 2013-08-05 10:26:15
59An Observational Look at Rotating Stars Stellar Structure and Evolution

An Observational Look at Rotating Stars Stellar Structure and Evolution

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Source URL: www.chara.gsu.edu

Language: English - Date: 2008-04-18 15:07:39
60E The Astrophysical Journal, 589:397–409, 2003 May 20

E The Astrophysical Journal, 589:397–409, 2003 May 20

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Source URL: www.aip.de

Language: English - Date: 2003-06-23 09:57:05