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Stellar physics
Results: 1072

#	Item
181	Chemical Physics Letters–154 www.elsevier.com/locate/cplett Absorption-spectral features of single-walled carbon nanotubes Yang Zhao, XiuJun Wang, Chi-Chiu Ma, GuanHua Chen Add to Reading List Source URL: yangtze.hku.hk Language: English - Date: 2010-12-19 08:35:08 Materials science Chemistry Carbon nanotube Nanomaterials Van Hove singularity Graphene Electronic band structure Density of states Stellar classification Physics Emerging technologies Condensed matter physics
182	Astronomy & Astrophysics A&A 555, L8DOI: Add to Reading List Source URL: www.aanda.org Language: English Galaxy formation and evolution Stellar evolution Astrophysics Galaxy Initial mass function Redshift Pea galaxy Pavel Kroupa Physical cosmology Astronomy Physics
183	The lithium content of Centauri Add to Reading List Source URL: www.aanda.org Language: English Astrophysics Stellar astronomy Dwarf galaxies Physical cosmology Local Group Star Sagittarius Dwarf Elliptical Galaxy Stellar classification Lithium Astronomy Physics Space
184	Institute of Astronomy, National Central University PHD QUALIFYING EXAMINATION — STELLAR ASTROPHYSICS 30th May, points) (a) (10 points) Write down the equations that describe the internal structure of star Add to Reading List Source URL: www.astro.ncu.edu.tw Language: English - Date: 2014-05-12 00:06:46 State functions Astrophysics Exotic matter Physical quantities White dwarf Degenerate matter Star formation Star Electron Physics Matter Stellar astronomy
185	Physics ± Uspekhi ± ) #2007 Uspekhi Fizicheskikh Nauk, Russian Academy of Sciences INSTRUMENTS AND METHODS OF INVESTIGATION Add to Reading List Source URL: selena.sai.msu.ru Language: English - Date: 2009-02-17 11:58:42 Observational astronomy Spectroscopy Vision Electromagnetic spectrum Color Astronomical spectroscopy Asteroid Stellar classification Reflectivity Electromagnetic radiation Physics Optics
186	PHD QUALIFY EXAMINATION — STELLAR ASTROPHYSICS 10th July, points) (a) Show that the outward pressure required to support a normal star of mass M and radius R is approximately M 2 G/R4 . In general the outw Add to Reading List Source URL: www.astro.ncu.edu.tw Language: English - Date: 2014-05-12 00:06:46 Stellar astronomy Astrophysics Space plasmas Physical phenomena Radiation pressure Eddington luminosity Star Photon Sun Physics Matter Light sources
187	PHD QUALIFY EXAMINATION — STELLAR ASTROPHYSICS 2nd March, points) An A type star has M = 2M , L = 12L , and Teﬀ = 8000 K. (a) Estimate its radius. Add to Reading List Source URL: www.astro.ncu.edu.tw Language: English - Date: 2014-05-12 00:06:46 Space Star Stellar structure Stellar evolution Virial theorem White dwarf Dyson sphere Stellar astronomy Physics Astronomy
188	Astronomy & Astrophysics A&A 569, L7DOI: Add to Reading List Source URL: www.aanda.org Language: English Space plasmas Science Sun Light sources Spectroscopy Corona Stellar classification Absorption spectroscopy Chromosphere Physics Chemistry Plasma physics
189	Astronomy & Astrophysics A&A 526, L6DOI: Add to Reading List Source URL: www.aanda.org Language: English Spectroscopy Emission spectroscopy Analytical chemistry Observational astronomy Star types Stellar classification Accretion disc Astronomical spectroscopy Balmer series Physics Chemistry Science
190	Convective plasma around solar pores S. Vargas Domínguez Abstract Magnetic structures are commonly observed in the solar photosphere at many different spatial scales, being sunspots and pores the most conspicuous ones. Add to Reading List Source URL: www.mssl.ucl.ac.uk Language: English - Date: 2010-04-20 07:47:25 Physics Space plasmas Plasma physics Stellar astronomy Sun Corona Hinode Velocity Proper motion Astronomy Light sources Space

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