'Effective temperature' presentation slideshows

Driving mechanism and energetic aspects of pulsations in g Doradus stars

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The chemical composition of MCP star HD 25354

643 views • 45 slides

Modelling of sprays using a customized version of FLUENT

647 views • 44 slides

Is the I nitial M ass F unction u niversal?

Is the I nitial M ass F unction u niversal?. Morten Andersen, M. R. Meyer, J. Greissl, B. D. Oppenheimer, M. Kenworthy, D. McCarthy Steward Observatory, University of Arizona, USA H. Zinnecker, AIP, Potsdam , Germany. Outline. Why study th e IMF? Why young clusters?

474 views • 35 slides

480 views • 31 slides

Heat Related Indices for the Health Sector

Heat Related Indices for the Health Sector. Glenn McGregor (University of Auckland, NZ) Christina Koppe (German Weather Service, Germany) Sari Kovats (London School of Hygiene and Tropical Medicine, UK). The Challenge of a Climate Index for the Health Sector.

404 views • 28 slides

The Sun

Goals: -Summarize the overall properties of the Sun. -Explain how energy travels from the solar core, through the interior, and out into space. -Name the Sun's outer layers and describe what those layers tell us about the Sun's surface composition and temperature.

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370 views • 25 slides

Seasonal Variations in the MINOS Far Detector

345 views • 23 slides

Di-lepton production in strongly coupled quark gluon plasma

Background and Motivation Di-lepton spectra from HIC Sensitivity to EOS Summary and conclusion arXiv: 1009.3091. Di-lepton production in strongly coupled quark gluon plasma. Jian Deng ( ?? ) USTC with Qun Wang, Nu Xu , Pengfei Zhuang 2010-10-19 ATHIC2010 @CCNU. We want to know.

332 views • 21 slides

How Massive are the First Stars? Statistical Study of the primordial star formation ? M popIII

334 views • 21 slides

ECSE-6230 Semiconductor Devices and Models I Lecture 6

ECSE-6230 Semiconductor Devices and Models I Lecture 6. Prof. Shayla Sawyer Bldg. CII, Rooms 8225 Rensselaer Polytechnic Institute Troy, NY 12180-3590 Tel. (518)276-2164 Fax. (518)276-2990 e-mail: sawyes@rpi.edu. March 13, 2014. sawyes@rpi.edu www.rpi.edu/~sawyes/courses.html . 1.

445 views • 19 slides

Precision Stellar astrophysics with song

Precision Stellar astrophysics with song. Marc Pinsonneault (OSU). Precision Stellar Astrophysics. New Era in Astronomy Seismology Large Surveys We can now measure things which have been assumed in stellar modeling Three specific examples: Helium Absolute metallicity Internal rotation.

304 views • 17 slides

Alan Robock Department of Environmental Sciences Rutgers University, New Brunswick, New Jersey USA

Lecture 6, 9/23/13. Climate Dynamics 11:670:461. Alan Robock Department of Environmental Sciences Rutgers University, New Brunswick, New Jersey USA. robock@envsci.rutgers.edu. http://envsci.rutgers.edu/~ robock. Stronger polar vortex Winter warming

256 views • 14 slides

ASCO WG on ozone cross sections

281 views • 14 slides

MAGNETARS AS COOLING NEUTRON STARS WITH INTERNAL HEATING

MAGNETARS AS COOLING NEUTRON STARS WITH INTERNAL HEATING. A.D. Kaminker , D.G. Yakovlev, A.Y. Potekhin, N. Shibazaki*, P. Sternin, and O.Y. Gnedin**. Ioffe Physical Technical Institute, St.-Petersburg, Russia *Rikkyo University, Tokyo 171-8501, Japan

249 views • 9 slides

Astronomy 340 Fall 2005

Astronomy 340 Fall 2005. Class #4 18 September 2007. Announcements. HW #1 due Thursday A little out of order Last time ? radiation (notes available today) This time ? tides. Solar Heating and Transport. Why? Astrophysics is all about how energy gets from point A to point B

170 views • 9 slides

Andrej Ficnar 1 , Steven S. Gubser 2 and Miklos Gyulassy 1

Shooting string holography of L ight quark jet quenching at RHIC and LHC. Andrej Ficnar 1 , Steven S. Gubser 2 and Miklos Gyulassy 1. 1 Department of Physics, Columbia University, New York, NY 10027, USA 2 Joseph Henry Laboratories, Princeton University, Princeton, NJ 08544, USA.

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Planetary Nebulae as tracers of SMC formation

1. THE DATA. 2. DETERMINATION OF AGE-ABUNDANCE RELATIONS. Planetary nebulae sample observed between 1999 and 2002. 1) Effective temperature ( T eff ). 2) Luminosity ( L/L ? ). of each PN central star. Object. Date. Site. E(B-V). Age derivation for PNe.

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K magnitude <= 15 mag J-H color in the range of 0.42 < J-H < 0.78.

1.37. A Survey of M star in the Field of View of Kepler Mahmoudreza Oshagh, Nader Haghighipour and Nuno C.Santos. Kepler 's public data Q0 and Q1. K magnitude <= 15 mag J-H color in the range of 0.42 < J-H < 0.78. H-K color in the range of 0.12 < H-K < 0.50. Proper Motion >= 0.108.

133 views • 1 slides