'Line strengths' presentation slideshows

Environmental and Industrial Measurements with Practical Laser Diagnostics

691 views • 64 slides

Assimilation of Infrared Radiance Observations

Assimilation of Infrared Radiance Observations. Will McCarty Global Modeling and Assimilation Office NASA Goddard Space Flight Center 2015 JCSDA Summer Colloquium 28 July 2015. What is Infrared Radiation?. What is Infrared Radiation?.

545 views • 54 slides

GRAVITATIONAL REDSHIFTS

766 views • 39 slides

3D Spectrography: II - The tracers

3D Spectrography: II - The tracers. Morphology : distribution of each component Dynamics : kinematics via the emission or absorption lines Line strengths : allow to study stellar populations. The different tracers: Gas. 90% H, 10% He Neutral, ionized, molecular. H. He. Dust. Mass.

608 views • 39 slides

Stellar Spectroscopy during Exoplanet Transits

357 views • 20 slides

Old Stellar Populations in Galaxy Clusters

Old Stellar Populations in Galaxy Clusters. Scott Trager (Kapteyn Institute, Groningen) with Sandy Faber (UCO/Lick) Alan Dressler (Carnegie Observatories). Introduction: Why Cluster Galaxies?. Why early-type galaxies?

366 views • 19 slides

Line-shapes and intensities of carbon monoxide transitions in the (3 0) band

175 views • 17 slides

Modeling X-Ray Photoionization Experiments Michael Rosenberg and David Cohen Swarthmore College

Modeling X-Ray Photoionization Experiments Michael Rosenberg and David Cohen Swarthmore College. Modeling Studies

153 views • 1 slides