'Interstellar clouds' presentation slideshows

The Discovery of C 60

The Discovery of C 60. ACS Philadelphia 2016. Rick atop Ap2. Ion Detector. Cluster Source. UV Laser Ionization. Cluster beam TOF mass spectrometer. Laser vaporization. Cluster beam source. Harry Kroto. Carbon Chain Molecules Found in Interstellar Clouds.

284 views • 28 slides

The study about the properties of the Gould Belt

432 views • 26 slides

Results from the High Elevation Antarctic Terahertz (HEAT) telescope on Ridge A

Results from the High Elevation Antarctic Terahertz (HEAT) telescope on Ridge A Craig Kulesa, on behalf of the HEAT and PLATO-R team. The Life Cycle of matter in the Galaxy remains poorly understood. some UV, X-rays. some UV, X-rays. 21 cm radio. ??. ??. visible light.

220 views • 21 slides

Star Formation and the Interstellar Medium

Star Formation and the Interstellar Medium. OBJECTIVES: Know the phases of star formation starting with the interstellar cloud. Understand how the life cycle of both low and high mass stars contribute to the makeup of the universe.

206 views • 20 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

396 views • 17 slides

Adventures with H 3 +

Adventures with H 3 +. Tom Geballe (Gemini Observatory) with thanks to: Takeshi Oka (U. Chicago) Ben McCall (U. Illinois), Miwa Goto (ESO- Garching ), Nick Indriolo (U. Michigan), Tomonori Usuda (Subaru Telescope) and the staffs of the

154 views • 15 slides

GALAXY

MILKY WAY. GALAXY. By: Eldrick Santos Cleon Molaer. GALAXY. Planets. Interstellar Clouds. Star Systems. PLANETS. INERSTELLAR CLOUDS. STAR SYSTEMS. TYPES OF GALAXIES. ANDROMEDA PINWHEEL SOMBRERO. ANDROMEDA GALAXY. PINWHEEL GALAXY. SOMBRERO GALAXY. SOURCES.

657 views • 11 slides

4 star formation

4 star formation. massive interstellar clouds. The galactic interstellar medium (ISM) consists of a roughly uniform gas with n ~10 5 atoms/m 3 . At current epoch, star formation takes place in massive interstellar clouds. Clouds have dimensions: R~10 pc, n ~5 10 9 atoms/m 3 , T~10 K.

264 views • 11 slides

Discuss the makeup of dark interstellar clouds

181 views • 8 slides

Nebulae!!! Interstellar clouds of Hydrogen, Helium, Ionized gases and Dust

Nebulae!!! Interstellar clouds of Hydrogen, Helium, Ionized gases and Dust.

103 views • 1 slides