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Slide 1November 8, 2008MWAM 081 The Implications of a High Cosmic-Ray Ionization Rate in Diffuse Interstellar Clouds Nick Indriolo, Brian D. Fields, Benjamin J. McCall University…
J. Astrophys. Astr. (1998) 19, 97–116 The Interstellar Clouds of Adams and Blaauw Revisited: An HI Absorption Study – I Jayadev Rajagopal, G. Srinivasan & Κ. S.…
The Implications of a High Cosmic-Ray Ionization Rate in Diffuse Interstellar Clouds Nick Indriolo, Brian D. Fields, Benjamin J. McCall University of Illinois at Urbana-Champaign…
Cosmic Neutrinos in IceCube Naoko Kurahashi Neilson University of Wisconsin, Madison IceCube Collaboration APS April Meeting – 4/7/2014 1 Highest energy particles observed…
Neumaier Clouds Yan Bulgak [email protected] October 30, MAR550, Challenger 165 Sets Defined by membership criterion: If A a set, then for all either or Fuzzy Sets Defined by…
Microsoft Word - 399-412.docJ. Astrophys. Astr. (1982) 3, 399–412 Interstellar Electron Density Μ. Vivekanand and R. Narayan Raman Research Institute, Bangalore
Dust.pptInterstellar Emission Why Dust • Dust attenuates and scatters UV/optical/NIR Amount of attenuation and spectral shape depends on dust properties (grain size/type)
NCTS(ISM)21Hiroyuki Hirashita ( ) ASIAA 1. ISM Composition/Phases 2. Interaction with Radiation 3. Multi-Phase ISM 4. Dynamical Processes 5. Summary Topics An ISM lecture
Slide 1 TEMPLATE DESIGN © 2008 www.PosterPresentations.com Total Amount Altitude Optical Depth Longwave High Clouds Shortwave High Clouds Shortwave Low Clouds Δ Optical…
3: Interstellar Absorption Lines: Radiative Transfer in the Interstellar Medium James R. Graham University of California, Berkeley AY 216 2 Interstellar Absorption Lines…
Magnetic Clouds and their Geoeffectiviness Cynthia López-Portela and Xochitl Blanco-Cano Instituto de Geofísica, UNAM A brief introduction: Magnetic Clouds’ characteristics…
Interactions SNR/MC Supernova remnants and molecular clouds Armand Fiasson LAPP - Annecy-le-vieux Where CRs originate? The usual suspects up to the knee are supernova remnants…
IIISupernovae 2016/09/16 arXiv: 1608.06689, doi: 10.1016/j.pss.2016.08.006 Light sources: OB stars (or RGs) - luminous (~ 105 Lsun) - UV (or IR) bright variation of extinction
Molecular Tracers of Turbulent Shocks in Molecular Clouds Molecular Tracers of Turbulent Shocks in Molecular Clouds Andy Pon, Doug Johnstone, Michael J. Kaufman ApJ, submitted…
Greek Research and Technology Network CIO Forum, 10/02/14 Ένα διεθνές λογισμικό για Clouds από Έλληνες μηχανικούς ICT Response to…
46 Warshavskoe shosse Moscow 115230 Russia ph: +7-499-678-2082 fax: +7-499-678-2083 web: wwwrmtltdru Copyright 2019 RMT Ltd The design and specifications of products can…
Diffuse interstellar bands λ5780 and λ5797 in the Antennae Galaxy as seen by MUSEAstronomy &Astrophysics Diffuse interstellar bands λ5780 and λ5797
1 Zadatak 081 Vedran, maturant Jedan kut u trokutu jednak je 2 3 drugog kuta i istodobno 4 5 trećeg. Koliki je najveći kut trokuta? Rješenje 081 Ponovimo! Zbroj kutova…
Slide 1 Astronomy 16: The Interstellar Medium 1 Evidence for the ISM How do we know there is an interstellar medium (ISM)? 1) The Oort Limit Hydrostatic equilibrium, but…