Singapore Air Final
Line Profiles Note - Figure obtained from lsa.atnos/SAElp05.htmlsa.atnos/SAElp05.htm.
Grop 9 Magnetics_powerpoint2015 Updated 17 4 15
Science With the Extreme-ultraviolet Spectrometer (EIS) on Solar-B by G. A. Doschek (with contributions from Harry Warren) presented at the STEREO/Solar-B.
Possible disk emission in the BLR of AGN Edi Bon Astronomical Observatory Belgrade, Serbia [email protected] L. Č. Popović 1, D. Ilić 2 1- Astronomical.
Astrophysics Yr 2 Session 6 Astronomical Spectroscopy.
Emission mechanisms. II GiorgioMatt Giorgio Matt (Dipartimento di Fisica, Università Roma Tre, Italy) Reference: Rybicki & Lightman, “Radiative processes.
High resolution (sub)millimetre studies of the chemistry of low-mass protostars Jes Jørgensen (CfA) Fredrik Schöier (Stockholm), Ewine van Dishoeck (Leiden),
Are inputs to standard solar models correct? OR The problem with solar abundances Sarbani Basu Yale Univesity.
1 Atmospheric dynamics of red supergiant stars Andrea Chiavassa Groupe de Recherche en Astronomie et Astrophysique du Languedoc GRAAL Thesis advisor: Bertrand.
Line Profiles of Magnetically Confined Winds Stephanie Tonnesen Swarthmore College.
Black Hole Physics with Constellation-X Chris Reynolds Department of Astronomy University of Maryland College Park.
