Polarimetry as a clue toward the nature of FeLoBAL quasars Daniel Lawther, Dark Cosmology Centre, Uni. of Copenhagen.
Aa17067 11
SN1014J in M82 A Pseudo-GOTOQ and what we can learn with really big telescopes and DIBs about QSOALS Donald G. York, Dan Welty, Jiaqi Jiang University.
UNM 29-Oct04 Galaxy-Halo Gas Kinematic Connection at 0.3 < z < 1 Collaborators: Chris Churchill (NMSU) Chuck Steidel (Caltech) Alice Shapley (Princeton)
Rand (2000) NGC 5775 Hα map. D = 24.8 Mpc It is an interacting galaxy.
The mass ratio of the stellar components of a spectroscopic binary can be directly computed from their ratio in radial velocities. To derive the total.
The planetary nebula M2-9: Balmer line profiles of the nuclear region Silvia Torres-Peimbert 1 Anabel Arrieta 2 Leonid Georgiev 1 1 Instituto de Astronomía,
The ELM Survey: A Targeted Search for the Most Extreme White Dwarf Binary Systems Alex Gianninas Astronomy Colloquium Wesleyan University February 25 th,
Spectropolarimetry of the starburst galaxy M82: Kinematics of dust outflow Michitoshi YOSHIDA 1),2), Koji S. KAWABATA 1), and Yoichi OHYAMA 3) 1) Hiroshima.
Water Fountains in Pre-Planetary Nebulae
Arp102B: An ADAF and a Torus ?
Abstract
