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Magnetic Fields & Turbulence in The Milky Way

Magnetic Fields & Turbulence in The Milky Way

Magnetic Fields & Turbulence in The Milky Way Bryan M. Gaensler Harvard-Smithsonian CfA + Marijke Haverkorn , Jo-Anne Brown , Natalya Bizunok, Naomi McClure-Griffiths, John Dickey, Anne Green The Magnetic Milky Way Galaxies are magnetic! (see review talk by Rainer Beck)

By niveditha
(375 views)

Chapter 14 Our Galaxy

Chapter 14 Our Galaxy

Chapter 14 Our Galaxy. 14.1 The Milky Way Revealed . Our Goals for Learning • What does our galaxy look like? • How do stars orbit in our galaxy?. Stars and planets are part of galactic ecosystem, within which the stars and planets are born, and recycled. What does our galaxy look like?.

By kuniko
(157 views)

Why Build Image Mosaics for Wide Area Surveys?

Why Build Image Mosaics for Wide Area Surveys?

An All-Sky 2MASS Mosaic Constructed on the TeraGrid. A. C. Laity, G. B. Berriman, J. C. Good (IPAC, Caltech); D. S. Katz, J. C. Jacob (JPL); L. Brieger, R. W. Moore (SDSC); R. Williams (Caltech); E. Deelman, G. Singh, M.-H. Su (ISI). Goals of the 2MASS All-Sky Mosaic Project.

By ailani
(83 views)

NuSTAR View of the Galactic Center: Chuck Hailey, Columbia University

NuSTAR View of the Galactic Center: Chuck Hailey, Columbia University

NuSTAR View of the Galactic Center: Chuck Hailey, Columbia University. Outline. Non-thermal filaments in the Galactic Center NuSTAR – Nuclear Spectroscopic Telescope Array NuSTAR’s view of the Galactic Center The Galactic Center at > 20 keV :

By emera
(138 views)

Protostars, nebulas and Brown dwarfs

Protostars, nebulas and Brown dwarfs

Protostars, nebulas and Brown dwarfs. Just before you meet with your black hole partner let’s talk a little more about protostars and star formation, use the following to enrich your posters on star formation.

By chipo
(146 views)

New View of Gas and Dust in the Solar Nebula

New View of Gas and Dust in the Solar Nebula

New View of Gas and Dust in the Solar Nebula. Measuring Oxygen in the Sun: Genesis Mission Results. New View of Gas and Dust in the Solar Nebula. Refractory inclusions (left) condensed from gas of solar composition with O-isotopes similar to the Sun (see Genesis data point).

By asis
(115 views)

GENESIS

GENESIS

GENESIS. SOLAR WIND. http://upload.wikimedia.org/wikipedia/commons/d/da/171879main_LimbFlareJan12_lg.jpg. OBJECTIVE. 18. 18. Ar. Ne. Argon. Neon. 39.948. 20.1797. http://upload.wikimedia.org/wikipedia/commons/7/76/Molecular.cloud.arp.750pix.jpg. MOLECULAR ClOUD.

By zuriel
(151 views)

ASTRONOMIC PICTURES

ASTRONOMIC PICTURES

ASTRONOMIC PICTURES. ASTRONOMIC PICTURES. ALICIA AGUADO PAREDES 1ºBACH B. ALICIA AGUADO PAREDES 1º BACH B. Aurora Over White Dome Geyser. 17 OCTOBER 2012.

By wynona
(119 views)

Astronomical Doomsday Scenarios

Astronomical Doomsday Scenarios

Astronomical Doomsday Scenarios. Comet and Asteroid Impacts. Impact of Comet Shoemaker-Levy on Jupiter. Impact of Comet Shoemaker-Levy on Jupiter. Impact of Comet Shoemaker-Levy on Jupiter. Major Impacts on Earth.

By presley
(94 views)

The Evolutionary Cycle of Stars

The Evolutionary Cycle of Stars

The Evolutionary Cycle of Stars. Cycle of Stars. The 3 major interests (or parameters) of astronomers are their mass, luminosity, their surface temperature & distance they are away from us.

By chase
(110 views)

Accreting isolated neutron stars

Accreting isolated neutron stars

Accreting isolated neutron stars. Magnetic rotator. Observational appearances of NSs (if we are not speaking about cooling) are mainly determined by P, Pdot, V, B, (also, probably by the inclination angle β ), and properties of the surrounding medium.

By milek
(93 views)

Where and How Are Massive Stars Formed in Isolation?

Where and How Are Massive Stars Formed in Isolation?

Where and How Are Massive Stars Formed in Isolation?. You-Hua Chu (U of Illinois) In collaboration with: R. Gruendl, R. Chen*, M. Gelman, M. Johnson (Illinois) H. Zinnecker (Potsdam). Galactic O-Type Stars. 70% in clusters or OB associations > 10% runaway stars

By adsila
(84 views)

Charge Exchange Models for X-ray Spectroscopy with AtomDB v2.0

Charge Exchange Models for X-ray Spectroscopy with AtomDB v2.0

Charge Exchange Models for X-ray Spectroscopy with AtomDB v2.0. Randall Smith, Adam Foster & Nancy Brickhouse Smithsonian Astrophysical Observatory. Building a CX model for X-ray Astrophysics. Back to basics!

By rad
(92 views)

SFUMATO: A self-gravitational MHD AMR code

SFUMATO: A self-gravitational MHD AMR code

SFUMATO: A self-gravitational MHD AMR code. Outflow. Circumstellar disk. Tomoaki Matsumoto ( Hosei Univerisity ). Matsumoto (2006) Submitted to PASJ, astro-ph/0609105. Magnetic field. Protostar. Computational domain is 1,000 times larger. H 13 CO + core.

By crevan
(165 views)

BBN Epoch: Evolution of Nuclear Composition

BBN Epoch: Evolution of Nuclear Composition

Первичный нуклеосинтез , образование D и содержание HD/H 2 в межзвездных облаках, существовавших 12 млрд. лет назад Д . А. Варшалович , А.В. Иванчик , С.А. Балашев Физико-технический институт им. А.Ф. Иоффе РАН 2009. BBN Epoch: Evolution of Nuclear Composition. t ~ 3-5 min

By knoton
(89 views)

IMAGES & MAPS

IMAGES & MAPS

By nakia
(57 views)

Hydrostatic Equilibrium and the Sun ’ s Core:

Hydrostatic Equilibrium and the Sun ’ s Core:

Hydrostatic Equilibrium and the Sun ’ s Core:. Clicker Question:. What does does ionized Helium, He II, contain? A: He nucleus only B: He nucleus and one electron C: He nucleus and two electrons D: He nucleus and three electrons. Rosette Nebula. Lagoon Nebula. Tarantula Nebula.

By keisha
(124 views)

1. Introduction

1. Introduction

2 Mar 2005, New trend WS. Evolution of CO molecule on dusts in dense core : formation of H 2 CO and CH 3 OH. Naoki Watanabe. Colleagues: A. Nagaoka, T. Shiraki, H. Hidaka, A. Kouchi. Institute of Low Temperature Science, Hokkaido Univ. 1. Introduction. 2. Experimental.

By janice
(114 views)

Multidimensional Models of Magnetically Regulated Star Formation

Multidimensional Models of Magnetically Regulated Star Formation

Multidimensional Models of Magnetically Regulated Star Formation. Shantanu Basu University of Western Ontario Collaborators: Glenn E. Ciolek (RPI), Takahiro Kudoh (NAO, Japan), Eduard I. Vorobyov (UWO). Submillimeter Astronomy, CfA, June 15, 2005. Taurus Molecular Cloud.

By indiya
(108 views)

VLA OH Zeeman Magnetic Field Detections Toward Five Galactic Supernova Remnants

VLA OH Zeeman Magnetic Field Detections Toward Five Galactic Supernova Remnants

VLA OH Zeeman Magnetic Field Detections Toward Five Galactic Supernova Remnants. C. L. Brogan 1 , D. A. Frail 2 , W. M. Goss 2 , & T. H. Troland 1. ( 1 University of Kentucky; 2 National Radio Astronomy Observatory).

By ivrit
(87 views)

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