ARMANINI Debris Flow
A measurement of_the_black_hole_mass_in_ngc_1097_using_alma
Der Paul van der Werf Leiden Observatory Radiative and mechanical feedback in the molecular gas in (U)LIRGs London September 16, 2011.
Star and Planet Formation
The hot core that is not a “Hot Core”: Orion KL Luis Zapata (MPIfR) Johannes Schmid-Burgk (MPIfR) Karl Menten (MPIfR) Max Planck Institut für Radioastronomie.
Star Formation and the GBT K-Band Focal Plane Array Crystal Brogan (NRAO/NAASC) T. R. Hunter (NRAO), C. J. Chandler (NRAO), K. Devine (U. Wisconsin), L.
Dust cycle through the ISM Francois Boulanger Institut d ’Astrophysique Spatiale Global cycle and interstellar processing Evidence for evolution Sub-mm.
Anomalous H 2 CO Absorption in the L1204/S140 Region and a Comparison with the CO (1-0) Emission Mónica I. Rodríguez 1,2, Laurent Loinard 1, Ron J. Allen.
HST/WFPC2 F606W
Susan CartwrightOur Evolving Universe1 Star Birth n Most of the bright stars we see have lifetimes much less than the age of the Solar System l l star.
Star Birth
