The H+ region contribution to [C II] 158- m emission
Open Access
- 26 April 2006
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 368 (4) , 1949-1958
- https://doi.org/10.1111/j.1365-2966.2006.10282.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 26 references indexed in Scilit:
- The H ii Region/PDR Connection: Self‐consistent Calculations of Physical Conditions in Star‐forming RegionsThe Astrophysical Journal Supplement Series, 2005
- Fine‐Structure Excitation of C+and Si+by Atomic HydrogenThe Astrophysical Journal, 2005
- The Dust Content and Opacity of Actively Star‐forming GalaxiesThe Astrophysical Journal, 2000
- Accurate Hydrogen Spectral Simulations with a Compact Model AtomThe Astrophysical Journal, 1997
- On the origin of the diffuse C(+) 158 micron line emissionThe Astrophysical Journal, 1994
- The photoelectric heating mechanism for very small graphitic grains and polycyclic aromatic hydrocarbonsThe Astrophysical Journal, 1994
- The interstellar medium in the starburst regions of NGC 253 and NGC 3256The Astrophysical Journal, 1994
- Physical conditions in the Orion Nebula and an assessment of its helium abundanceThe Astrophysical Journal, 1991
- The relationship between infrared, optical, and ultraviolet extinctionThe Astrophysical Journal, 1989
- IRAS observations of galaxies in the Virgo cluster areaThe Astrophysical Journal Supplement Series, 1988