'Interstellar gas' presentation slideshows

Chapter 6 Formation of Planetary Systems: Our Solar System and Beyond

Chapter 6 Formation of Planetary Systems: Our Solar System and Beyond. 6.1 A Brief Tour of the Solar System. Our goals for learning: What does the solar system look like?. What does the solar system look like?. The solar system exhibits clear patterns of composition and motion.

1.06k views • 105 slides

Chapter 6 Formation of Planetary Systems Our Solar System and Beyond

Chapter 6 Formation of Planetary Systems Our Solar System and Beyond. The solar system exhibits clear patterns of composition and motion. These patterns are far more important and interesting than numbers, names, and other trivia. Planets are very tiny compared to distances between them. Sun.

894 views • 66 slides

Astro 300B: Jan. 26, 2011 Thermal radiation and Thermal Equilibrium

Astro 300B: Jan. 26, 2011 Thermal radiation and Thermal Equilibrium. Thermal Radiation, and Thermodynamic Equilibrium. Thermal radiation is radiation emitted by matter in thermodynamic equilibrium.

888 views • 62 slides

Galaxies Galaxies M81

641 views • 44 slides

A Star Is Born

603 views • 44 slides

The Milky Way Galaxy

530 views • 39 slides

Discovering the Universe Ninth Edition

564 views • 39 slides

LECTURE 17, OCTOBER 28, 2010

LECTURE 17, OCTOBER 28, 2010. ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu. Question 1. a) there are no stars there. b) stars in that direction are obscured by interstellar gas . c) stars in that direction are obscured by interstellar dust .

469 views • 37 slides

LECTURE 17, OCTOBER 28, 2010

LECTURE 17, OCTOBER 28, 2010. ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu. Question 1. a) there are no stars there. b) stars in that direction are obscured by interstellar gas . c) stars in that direction are obscured by interstellar dust .

458 views • 37 slides

Interstellar Magnetic Fields in the Solar Vicinity

443 views • 35 slides

Andrzej Radosz Institute of Physics Wroclaw University of Technology aradosz@if.pwr.wroc.pl

918 views • 33 slides

OTHER TELESCOPES

OTHER TELESCOPES. OTHER TELESCOPES. Radio telescopes Fundamental design similar to optical telescopes. Made up of large dishes to accommodate longer wavelengths of electromagnetic radiation. Bowl-shaped surface is crafted of steel and wire mesh. . Radio Telescopes.

472 views • 31 slides

Chapter 18 The Interstellar Medium

Chapter 18 The Interstellar Medium. Units of Chapter 18. 18.1 Interstellar Matter 18.2 Emission Nebulae 18.3 Dark Dust Clouds 18.4 21-Centimeter Radiation 18.5 Interstellar Molecules. 18.1 Interstellar Matter.

501 views • 31 slides

291 views • 18 slides

Active Galactic Nuclei

Active Galactic Nuclei. 4C15 - High Energy Astrophysics emp@mssl.ucl.ac.uk http://www.mssl.ucl.ac.uk/. Introduction. Apparently stellar Non-thermal spectra High redshifts Seyferts (usually found in spiral galaxies) BL Lacs (normally found in ellipticals)

300 views • 17 slides

ISM & Astrochemistry Lecture 1

ISM & Astrochemistry Lecture 1. Interstellar Matter. Astrochemistry is the study of the synthesis of molecules in space and their use in determining the properties of Interstellar Matter, the material between the stars. Comprises Gas and Dust

395 views • 17 slides

170 views • 16 slides

MIR Diagnostics and Molecular Gas in Local Luminous Infrared Galaxies

MIR Diagnostics and Molecular Gas in Local Luminous Infrared Galaxies . Andreea Petric Collaborators: L. Armus, J. Howell, J. Surace (SSC/Caltech), A. Evans (UVA) J. Mazzarella, D. Frayer, T. Vavilkin, C. Bridge (IPAC) P. Appleton (IPAC), D. Sanders, J. Barnes, (IFA)

345 views • 15 slides

Stellar Evolution

Star Formation. Stellar Evolution. 1) Nebula. Cloud of interstellar gas and dust Collapses due to its own gravity Begins Star Formation. 2) Protostar. Rotating disk shape Hot condensed object at the center Fusion begins. 3) Main Sequence Star. Fusing Hydrogen into Helium

276 views • 13 slides

Radio Waves Interaction With Interstellar Matter

Radio Waves Interaction With Interstellar Matter. A cosmic journey brought to you by McGourty-Rideout. Interstellar Medium. Gaseous - almost all hydrogen H I- neutral hydrogen one proton and one electron( most) H II ionized hydrogen- - no electron just a proton - near hot stars

333 views • 8 slides