Turbulence as a Unifying Principle in Coronal Heating and Solar/Stellar Wind Acceleration Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics.
1. Introduction Her X-1 is an eclipsing binary system, with a neutron star (NS) primary and an A/F secondary star. The spin period is ~1.24 s and the orbital.
Models of the 5-Minute Oscillation & their Excitation Bob Stein – Michigan State U. 1.
Crushing of interstellar gas clouds Part I - Thermal Conduction and Radiative Losses - Equations: Heat Flux: Initial conditions Cloud Mass Fraction: choose.
X-ray flare on the single giant HR 9024 David Garcia-Alvarez (CfA) David Huenemoerder (MIT) Jeremy Drake (CfA) Fabio Reale (Univ. Palermo) Paola Testa.
X-ray flare on the single giant HR 9024
X-ray Observation of Accretion Disk in AGN
Crushing of interstellar gas clouds Part I - Thermal Conduction and Radiative Losses -
Taking the fingerprints of stars, galaxies, and interstellar gas clouds Absorption and emission from atoms, ions, and molecules.
Can magnetic waves in aurorae transform into acoustic waves? Jada Maxwell & E.J. Zita, The Evergreen State College, Olympia, WA 98505 Contact: Jada Maxwell,
2001/3/30 1 X-ray Observation of Accretion Disk in AGN K. Hayashida (Osaka University)
The Large Quasar Astrometric Catalogue (LQAC) and the densification of the ICRF through the Large Quasar Reference Frame (LQRF) J.Souchay, C.Barache,S.Bouquillon,A.H.Andrei,F.Taris.