Observational Consequences of Fine‐Structure Line Optical Depths on Infrared Spectral Diagnostics-Reference-Cited by-同舟云学术

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Observational Consequences of Fine‐Structure Line Optical Depths on Infrared Spectral Diagnostics

Published:2003-02 Issue:804 Volume:115 Page:188-192
ISSN:0004-6280
Container-title:Publications of the Astronomical Society of the Pacific
language:en
Short-container-title:PUBL ASTRON SOC PAC

Author:

Abel Nicholas,Bryant Adam,Dhakal Prabodh,Gale Ashley,Gibson Alva,Goddard William,Howard Chad,Kolarkar Ameya,Lim Pey Lian,Shaw Gargi,Ferland Gary

Publisher

IOP Publishing

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference15 articles.

1. Emission‐Line Helium Abundances in Highly Obscured Nebulae

2. Physical conditions in the Orion Nebula and an assessment of its helium abundance

3. Luminosity Indicators in Dusty Photoionized Environments

4. High-Resolution Optical and Ultraviolet Absorption-Line Studies of Interstellar Gas

5. Ferland, G. J. 2002, Hazy, a Brief Introduction to Cloudy (Univ. Kentucky Dept. Phys. Astron. Int. Rep.)

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1. Exploring the hardness of the ionising radiation with the infrared softness diagram;Astronomy & Astrophysics;2024-03-29

2. DUST-BOUNDED ULTRALUMINOUS INFRARED GALAXIES: MODEL PREDICTIONS FOR INFRARED SPECTROSCOPIC SURVEYS;The Astrophysical Journal;2009-07-30

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