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Main sequence
Results: 126

#	Item
41	From Young and Hot to Old and Cold: Comparing White Dwarf Cooling Theory to Main Sequence Stellar Evolution in Open Clusters arXiv:astro-phv1 14 Feb 2005 Add to Reading List Source URL: www.as.utexas.edu Language: English - Date: 2005-11-04 13:01:45 Physical cosmology Astrophysics Star clusters Globular cluster NGC objects Galaxy Star Cosmic distance ladder Hyades Astronomy Space Stellar astronomy
42	Individual patient positioning document Patient ID: Date: o E1 Add to Reading List Source URL: www.orfit.com Language: English - Date: 2014-11-17 05:14:13 O-type main-sequence star Neurotoxins Military insignia Maitotoxin
43	All SEM doctors are now required to undergo a yearly appraisal under the auspices of the Faculty of Sports & Exercise Medicine Add to Reading List Source URL: www.fsem.ac.uk Language: English - Date: 2013-01-07 10:41:20 Neurotoxins Military insignia O-type main-sequence star
44	Astronomy 1011H: Astronomy 1011H Web Site: Professor Paul Woodward: Add to Reading List Source URL: www.lcse.umn.edu Language: English - Date: 2015-04-09 21:14:55 Star types Astrophysics Stellar astronomy Light sources Hertzsprung-Russell classifications Star Asymptotic giant branch White dwarf Main sequence Astronomy Stellar evolution Space
45	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 Add to Reading List Source URL: www.astro.ncu.edu.tw Language: English - Date: 2014-05-12 00:06:46 Stellar evolution Space Stellar astronomy Light sources Hertzsprung-Russell classifications Star White dwarf Nuclear fusion Main sequence Astronomy Physics Star types
46	MAIN SEQUENCE WARM-UP POSES home practice Add to Reading List Source URL: www.yogajournal.com.au Language: English - Date: 2013-12-02 17:36:40 Human anatomy Uttanasana Balasana Surya Namaskara Adho Mukha Svanasana Turn Sitting Sirsasana USAG compulsory routines Asanas Human behavior Buddhist meditation
47	Institute of Astronomy, National Central University PHD QUALIFYING EXAMINATION — STELLAR ASTROPHYSICS 28th May, points) A model star of mass M has a density distribution ρ = ρc [1 − (r/R)a ], where a > Add to Reading List Source URL: www.astro.ncu.edu.tw Language: English - Date: 2014-05-12 00:06:46 Physics Stellar evolution Astrophysics Exotic matter Stellar astronomy White dwarf Star Main sequence Stellar classification Astronomy Star types Matter
48	PhD Qualifying Exam (2010) --- 星球天文物理 What is limb darkening? Can the limb darkening be seen if the star were isothermal, that is, the temperature is a constant all over the star? Why? Finally, explain how t Add to Reading List Source URL: www.astro.ncu.edu.tw Language: English - Date: 2014-05-12 00:06:46 Space Star Luminosity Eddington luminosity Sun Main sequence Limb darkening Temperature Jeans instability Physics Astronomy Astrophysics
49	Exercise: Draw HR Diagram of Star Cluster VerExercise: Draw HR Diagram of Star Cluster Guide for Teachers INDEX Add to Reading List Source URL: paofits.nao.ac.jp Language: English - Date: 2012-03-25 00:43:47 Space Hertzsprung-Russell classifications Stellar astronomy Standard candles Hertzsprung–Russell diagram Globular cluster Star Main sequence Horizontal branch Astronomy Star types Stellar evolution
50	Astronomy & Astrophysics A&A 564, L7DOI: Add to Reading List Source URL: www.aanda.org Language: English Space Stellar astronomy Universe Dorado constellation Large Magellanic Cloud Tarantula Nebula Herbig Ae/Be star Stellar classification Pre-main-sequence star Astronomy Star types Star formation

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