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Massive Star Formation under Different Z & Galactic Environment Rosie Chen (University of Virginia) Remy Indebetouw, You-Hua Chu, Robert Gruendl, Gerard Testor, &…

Centro de Radioastronomía y Astrofísica, UNAM Massive Massive Star Formation Introduction The paradigm for low-mass star formation The search for jets and disks in massive…

THE COEVOLUTION OF NUCLEAR STAR CLUSTERS, MASSIVE BLACK HOLES, AND THEIR HOST GALAXIES Fabio Antonini1, Enrico Barausse2,3, and Joseph Silk2,3,4,5 1 Center for Interdisciplinary…

A young massive planet in a star-disk system Setiawan, Henning, Launhardt et al. January 2008, Nature Letter 451 ESO Journal Club – January 2008 The target: TW Hya Spec.…

Slide 1 X-ray Emission and Absorption in Massive Star Winds Constraints on shock heating and wind mass-loss rates David Cohen Swarthmore College What we know about X-rays…

“Formation histories of galactic halos via chemical abundance analyses of near-by stellar systems” Small-scale heros: massive-star enrichment in ultrafaint dSphs Andreas…

Slide 1 X-ray Emission and Absorption in Massive Star Winds Constraints on shock heating and wind mass-loss rates David Cohen Swarthmore College What we know about X-rays…

l 2 00 5 Massive Star Birth: A Crossroads of Astrophysics Proceedings IAU Symposium No. 227, 2005 E.B. Churchwell, M. Felli & C.M. Wadsley, eds. c© 2005 International

Trigonometric parallax observations of water masers Katharina Immer 05.12.2012 Introduction Observations Results Summary Massive Star Formation Although massive stars have

Earth Science Notes Stars and Galaxies What is a Star? A star is a massive, luminous ball of plasma that is held together by gravity. Stars shines due to nuclear fusion in…

Massive Star Formation in the Galactic Center By Don F. F i g e r Rochester Institute of Technology, Rochester, NY, USA The Galactic center is a hotbed of star formation…

Astronomy Astrophysics manuscript no n2hp_mapping c©ESO 2014 January 9 2014 Kinematic structure of massive star-forming regions - I Accretion along filaments J Tackenberg1…

Massive Star Evolution overview Michael Palmer Intro - Massive Stars Massive stars M > 8Mo Many differences compared to low mass stars, ex: Lifetime Dominate energy production…

1. Astronomy & Astrophysics manuscript no. aa21771-13 c ESO 2014 May 12, 2014 A VLT/FLAMES survey for massive binaries in Westerlund 1 IV. Wd1-5 – binary…

Massive star feedback – from the first stars to the present Jorick Vink (Imperial College London, UK) Outline Why predict dM/dt ? (as a function of Z?) Methods: CAK &…

Sgr B2  Cluster of Massive Stars. No10: Associated to UC HII regions No13: No association to UC HII regions No13  No10 Total Lx~1033 erg/s   Each Lx~ 1032 erg/s…

A review of maser polarizationi and magnetic fields Maser Polarization and Magnetic fields during Massive Star Formation W. H. T. Vlemmings ASP Conference Series, Vol. 387,…

ar X iv :0 81 1. 06 79 v1 [ as tr o- ph ] 5 N ov 2 00 8 2008 October 29 Trigonometric Parallaxes of Massive Star Forming Regions: II. Cep A & NGC 7538 L. Moscadelli1,…

GAMA From little blue fuzzies to massive red monsters The epoch of  star  formation  for  the  most  massive galaxies Sarah Brough (AAO) Executive Summary…

Massive star feedback – from the first stars to the present Jorick Vink (Keele University) Outline Why predict Mass-loss rates? (as a function of Z) Monte Carlo Method…