Hertzsprung

Results: 93



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21Astronomy & Astrophysics manuscript no. P02a (DOI: will be inserted by hand later) July 1, 2003  Radiation-driven winds of hot luminous stars

Astronomy & Astrophysics manuscript no. P02a (DOI: will be inserted by hand later) July 1, 2003 Radiation-driven winds of hot luminous stars

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Source URL: www.usm.uni-muenchen.de

Language: English - Date: 2003-07-01 13:01:36
22

PDF Document

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Source URL: science.uniserve.edu.au

Language: English - Date: 2012-04-30 00:35:09
23Asteroseismology of Red Horizontal Branch Variables in M4 - K2/C2 proposal Charles Kuehn1, Robert Szabó2, Karen Kinemuchi3, Timothy Bedding1, Dennis Stello1 1 University of Sydney, Australia, 2Konkoly Observatory, Hunga

Asteroseismology of Red Horizontal Branch Variables in M4 - K2/C2 proposal Charles Kuehn1, Robert Szabó2, Karen Kinemuchi3, Timothy Bedding1, Dennis Stello1 1 University of Sydney, Australia, 2Konkoly Observatory, Hunga

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Source URL: keplerscience.arc.nasa.gov

Language: English - Date: 2015-04-02 16:37:16
24Evolution of solar mass star past main sequence (a review). Many were confused, so worth a recap. Core and burning shells right near it drive the dynamics. Outer layers are passive, except insofar as their weig

Evolution of solar mass star past main sequence (a review). Many were confused, so worth a recap. Core and burning shells right near it drive the dynamics. Outer layers are passive, except insofar as their weig

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Source URL: www.lcse.umn.edu

Language: English - Date: 2015-04-06 21:03:56
25Microsoft Word - JSS_david_van_dyk_12_marc_2010.doc

Microsoft Word - JSS_david_van_dyk_12_marc_2010.doc

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Source URL: www.bm.ust.hk

Language: English - Date: 2010-03-04 03:15:24
26BIOGRAPHIES  mo EjNAR H E R T Z S P R U N G

BIOGRAPHIES mo EjNAR H E R T Z S P R U N G

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Source URL: www.dwc.knaw.nl

Language: English - Date: 2014-09-02 07:30:27
27A  The Astrophysical Journal, 632:266–276, 2005 October 10 # 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.  DEEP PHOTOMETRY OF THE GLOBULAR CLUSTER M5: DISTANCE ESTIMATES

A The Astrophysical Journal, 632:266–276, 2005 October 10 # 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A. DEEP PHOTOMETRY OF THE GLOBULAR CLUSTER M5: DISTANCE ESTIMATES

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Source URL: www.as.utexas.edu

Language: English - Date: 2006-01-30 17:38:47
28Astronomy 1011H:  Astronomy 1011H Web Site: Professor Paul Woodward:

Astronomy 1011H: Astronomy 1011H Web Site: Professor Paul Woodward:

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Source URL: www.lcse.umn.edu

Language: English - Date: 2015-04-09 21:14:55
29PHD QUALIFY EXAMINATION — STELLAR ASTROPHYSICS March, points) A low mass sequence star has mass M , radius R and effective surface temperature Teff . (a) (15 points) Find the average time a photon reside

PHD QUALIFY EXAMINATION — STELLAR ASTROPHYSICS March, points) A low mass sequence star has mass M , radius R and effective surface temperature Teff . (a) (15 points) Find the average time a photon reside

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Source URL: www.astro.ncu.edu.tw

Language: English - Date: 2014-05-12 00:06:46
30Microsoft Word - qual2009

Microsoft Word - qual2009

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Source URL: www.astro.ncu.edu.tw

Language: English - Date: 2014-05-12 00:06:46