1 / 14

The Interstellar Medium

The Interstellar Medium. ISM Properties - 99% is gas, mostly H, He - about 1 atom/cm 3 - 1% is dust grains, mostly C, ices of water, ammonia, methane - 10 -6 meters in diameter - about 1 grain/100m 3. ISM Properties (continued) - Temps between 5K to 10,000K near hot stars

odysseus
Télécharger la présentation

The Interstellar Medium

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. The Interstellar Medium

  2. ISM Properties - 99% is gas, mostly H, He - about 1 atom/cm3 - 1% is dust grains, mostly C, ices of water, ammonia, methane - 10-6 meters in diameter - about 1 grain/100m3

  3. ISM Properties (continued) - Temps between 5K to 10,000K near hot stars - About 10% of the mass of our Galaxy is ISM

  4. HII regions - ionized regions around hot stars Ionized H (HII) Hot O,B star

  5. 30 Doradus (Trantula Nebula)

  6. The ISM absorbs short wavelengths more than long ones -> the ISM reddens and dims starlight

  7. 21-cm Radiation H-Atom Low energy High Energy 21 cm photon

  8. Nebulae (clouds) - Concentrations in the ISM (1,000’s of atoms/cm3) - The building blocks of the Stars

  9. Dark Nebulae - lots of Dust Horsehead Nebula

  10. Keyhole Nebula

  11. Reflection Nebulae - shine by reflected light from nearby stars Witch Head Nebula

  12. Orion Nebula

  13. Trifid Nebula

More Related