(Q68799841)

Kramer C.

3

1 reference

Kraemer K.

4

1 reference

Stutzki J.

5

1 reference

Mookerjea B.

6

1 reference

language of work or name

English

0 references

publication date

2003

1 reference

Astronomy and Astrophysics

published in

1 reference

volume

406

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page(s)

915–935

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Structure and evolution of molecular clouds near H II regions. II. The disk constrained H II region, S 106

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COBE far infrared absolute spectrophotometer observations of galactic lines

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The abundances of atomic carbon and carbon monoxide compared with visual extinction in the Ophiuchus molecular cloud complex

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Anatomy of a region of star formation: infrared images of S 106 (AFGL 2584)

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Atomic carbon in galaxies

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CO lines toward NGC 2024 and other star-forming regions : a closer look at the warm gas component

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Submillimeter and millimeter observations of jupiter

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Submillimeter and far-infrared spectroscopy of M 17 and S 106: UV-heated, quiescent molecular gas ?

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The S106 star-forming region

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Low-density photodissociation regions

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Parsec-scale penetration of ultraviolet photons into molecular clouds : CII 158 micron mapping of W 3, NGC 1977 and NGC 2023

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CI and CO in the spiral galaxies NGC 6946 and M 83

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Large-scale mapping observations of the C I (^3^P_1_-^3^P_0_) and CO (J = 3-2) lines toward the Orion A molecular cloud

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Warm dense gas in luminous protostellar regions: a submillimeter and far-infrared CO line study

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12C/13C isotope ratio across the galaxy from observations of 13C18O in molecular clouds

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Observations of an expanding molecular ring in S 106

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Far-infrared observations of M17SW : the clumpy structure of the photodissociation region

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Large‐Scale CiEmission from Molecular Clouds with Associated Ultraviolet Sources

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Large-scale ^13^CO J=5-->4 and [C I] mapping of Orion A

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The molecular environment of S 106 IR

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A multiwavelength study of the S106 region. I. Structure and dynamics of the molecular gas

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Thermal infrared imaging of the bipolar H II region S106

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The bipolar nebula S 106 : photometric polarimetric, and spectropolarimetric observations

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The 158 micron C II line: a measure of global star formation activity in galaxies

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The optical depth of the 158 micron [12CII] line: detection of the F = 1->0 [13C II] hyperfine-structure component

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The infrared response of molecular hydrogen gas to ultraviolet radiation: high-density regions

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Submillimeter and far-infrared line observations of M 17 SW: a clumpy molecular cloud penetrated by ultraviolet radiation

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Anatomy of a photodissociation region : high angular resolution images of molecular emission in the Orion bar

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