Xray and protostars_in_the_trifid_nebula
An eclipsing binary_distance_to_the_large_magellanic_cloud_accurate_to_two_per_cent
Most Stars Are Single ! C. J. Lada ApJ, 640, L63 (2006) 1.From observations: a low binary fraction for late-type stars 2.2/3 of all disk MS stellar systems.
Convective Dynamos and the Minimum X-ray Flux in Solar-Type Main Sequence Stars D. J. Bercik 1, G. H. Fisher 1, C. M. Johns-Krull 2, & W. P. Abbett 1 1.
M2FS: Michigan/Magellan Fiber System. M2FS (Michigan/Magellan Fiber System) Fiber-fed MOS w/2 independent and identical spectrograph arms 256 total fibers.
6 th IRAM 30m Summer School Star formation near and far A. Fuente Observatorio Astronómico Nacional (OAN, Spain) Photon Dominated Regions I. Physical conditions.
Steve Drake HEASARC/GSFC & USRA/CRESST
MPIfR Colloquium, 23 April 2004 Yoshiaki Hagiwara ASTRON Collaborators: P.J.Diamond, W.A. Sherwood, W. Baan, N.Nakai M.Miyoshi, C.Henkel, E.Rovilos, K.Hachisuka.
Angular momentum transport and mixing in rotating stars
X-ray Universe 2011 The High-Energy Environment of Extrasolar Planets J. Schmitt Hamburger Sternwarte Email: [email protected] Internet: .
6 th IRAM 30m Summer School Star formation near and far
