H 2 EXCITATION STRUCTURE ON THE SIGHTLINES TO δ SCORPII AND ζ OPHIUCI: FIRST RESULTS FROM THE SUB-ORBITAL LOCAL INTERSTELLAR CLOUD EXPERIMENT-Reference-Cited by-同舟云学术

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H 2 EXCITATION STRUCTURE ON THE SIGHTLINES TO δ SCORPII AND ζ OPHIUCI: FIRST RESULTS FROM THE SUB-ORBITAL LOCAL INTERSTELLAR CLOUD EXPERIMENT

Published:2013-07-08 Issue:1 Volume:772 Page:L9
ISSN:2041-8205
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

France Kevin,Nell Nicholas,Kane Robert,Burgh Eric B.,Beasley Matthew,Green James C.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.1088/2041-8205/772/1/L9/pdf

Reference37 articles.

1. A far UV study of interstellar gas towards HD 34078: High excitation H2 and small scale structure

2. Hopkins Ultraviolet Telescope observations of H2 toward the planetary nebula NGC 1535

3. Inferring Physical Conditions in Interstellar Clouds of H2

4. Direct Measurement of the Ratio of Carbon Monoxide to Molecular Hydrogen in the Diffuse Interstellar Medium

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1. CHESS: An innovative concept for high-resolution, far-UV spectroscopy;Experimental Astronomy;2020-10-01

2. Revisiting the Temperature of the Diffuse ISM with CHESS Sounding Rocket Observations;The Astrophysical Journal;2019-06-17

3. The fourth flight of CHESS: spectral resolution enhancements for high-resolution FUV spectroscopy;Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray;2018-07-06

4. Digital micromirror array enabled integral field spectroscopy for far-ultraviolet astronomy;MOEMS and Miniaturized Systems XVII;2018-02-22

5. The third flight of the Colorado high-resolution echelle stellar spectrograph (CHESS): improvements, calibrations, and preliminary results;UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XX;2017-08-29

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