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Documents Chapter 17 Quasars and Active Galaxies. Introduction Quasars, and the way in which they became...

Slide 1Chapter 17 Quasars and Active Galaxies Slide 2 Introduction Quasars, and the way in which they became understood, have been one of the most exciting stories of the…

Science Multiwavelength observations...

arX iv: 15 02 .01 79 4v 2 [as tro -ph .SR ] 2 6 F eb 20 15 Mon. Not. R. Astron. Soc. 000, 1–?? (2002) Printed 27 February 2015 (MN LATEX style file v2.2) Multiwavelength…

Documents Francesco Damiani Young Clusters in the Gaia-ESO Survey, Palermo, 20 May 2014 Francesco Damiani...

Slide 1 Francesco Damiani Young Clusters in the Gaia-ESO Survey, Palermo, 20 May 2014 Francesco Damiani INAF-Osservatorio Astronomico di Palermo, ITALY Stellar classification…

Documents Magnetism and Rotation in Herbig Ae/Be stars E. Alecian Laboratoire d’Astrophysique de...

Slide 1Magnetism and Rotation in Herbig Ae/Be stars E. Alecian Laboratoire d’Astrophysique de l’Observatoire de Grenoble In collaboration with G.A. Wade, C. Catala, C.…

Documents Stellar Atmospheres: Emission and Absorption 1 Emission and Absorption

Slide 1 Stellar Atmospheres: Emission and Absorption 1 Emission and Absorption  Slide 2 Stellar Atmospheres: Emission and Absorption 2 Chemical composition Stellar atmosphere…

Documents June 06, 2013 Putting A Stars into Context: Evolution, Environment, and Related Stars Observational....

June 06, 2013 Putting A Stars into Context: Evolution, Environment, and Related Stars Observational Studies of roAp Stars Mikhail Sachkov Institute of Astronomy RAS, Moscow…

Documents Observational Studies of roAp Stars

June 06, 2013 Putting A Stars into Context: Evolution, Environment, and Related Stars Observational Studies of roAp Stars Mikhail Sachkov Institute of Astronomy RAS, Moscow…

Documents Automated Fitting of High-Resolution Spectra of HAeBe stars Improving fundamental parameters Jason.....

Automated Fitting of High-Resolution Spectra of HAeBe stars Improving fundamental parameters Jason Grunhut Queenâs University/RMC Motivation Common ways to determine temperature…

Documents The Stellar Zoo

The Stellar Zoo Weird stars across the HR diagram What causes stellar abundance anomalies? The Upper Upper Main Sequence 100 (or so) solar masses, T~20,000 â 50,000 K Luminosities…

Documents Astronomical Surveys

DIGITIZATION OF THE FBS: ITS FUTURE USE AND EXPECTED RESULTS Large Astronomical Surveys, Databases, and Archives Areg Mickaelian, Byurakan Astrophysical Observatory (BAO)…