ui.adsabs.harvard.edu/abs/1997ApJS..111..387C/abstract

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https://ui.adsabs.harvard.edu/abs/1997ApJS..111..387C/abstract

The High-Resolution IRAS Galaxy Atlas

An atlas of the Galactic plane (-4.7d < b < 4.7d), along with the molecular clouds in Orion, ρ Oph, and Taurus-Auriga, has been produced at 60 and 100 μm from IRAS data. The atlas consists of resolution-enhanced co-added images with 1'-2' resolution and co-added images at the native IRAS resolution. The IRAS Galaxy Atlas, together with the Dominion Radio Astrophysical Observatory H I line/21 cm continuum and FCRAO CO (1-0) Galactic plane surveys, which both have similar (~1') resolution to the IRAS atlas, provides a powerful tool for studying the interstellar medium, star formation, and large-scale structure in our Galaxy. This paper documents the production and characteristics of the atlas.



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The High-Resolution IRAS Galaxy Atlas

https://ui.adsabs.harvard.edu/abs/1997ApJS..111..387C/abstract

An atlas of the Galactic plane (-4.7d < b < 4.7d), along with the molecular clouds in Orion, ρ Oph, and Taurus-Auriga, has been produced at 60 and 100 μm from IRAS data. The atlas consists of resolution-enhanced co-added images with 1'-2' resolution and co-added images at the native IRAS resolution. The IRAS Galaxy Atlas, together with the Dominion Radio Astrophysical Observatory H I line/21 cm continuum and FCRAO CO (1-0) Galactic plane surveys, which both have similar (~1') resolution to the IRAS atlas, provides a powerful tool for studying the interstellar medium, star formation, and large-scale structure in our Galaxy. This paper documents the production and characteristics of the atlas.



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https://ui.adsabs.harvard.edu/abs/1997ApJS..111..387C/abstract

The High-Resolution IRAS Galaxy Atlas

An atlas of the Galactic plane (-4.7d < b < 4.7d), along with the molecular clouds in Orion, ρ Oph, and Taurus-Auriga, has been produced at 60 and 100 μm from IRAS data. The atlas consists of resolution-enhanced co-added images with 1'-2' resolution and co-added images at the native IRAS resolution. The IRAS Galaxy Atlas, together with the Dominion Radio Astrophysical Observatory H I line/21 cm continuum and FCRAO CO (1-0) Galactic plane surveys, which both have similar (~1') resolution to the IRAS atlas, provides a powerful tool for studying the interstellar medium, star formation, and large-scale structure in our Galaxy. This paper documents the production and characteristics of the atlas.

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      An atlas of the Galactic plane (-4.7d < b < 4.7d), along with the molecular clouds in Orion, ρ Oph, and Taurus-Auriga, has been produced at 60 and 100 μm from IRAS data. The atlas consists of resolution-enhanced co-added images with 1'-2' resolution and co-added images at the native IRAS resolution. The IRAS Galaxy Atlas, together with the Dominion Radio Astrophysical Observatory H I line/21 cm continuum and FCRAO CO (1-0) Galactic plane surveys, which both have similar (~1') resolution to the IRAS atlas, provides a powerful tool for studying the interstellar medium, star formation, and large-scale structure in our Galaxy. This paper documents the production and characteristics of the atlas.
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      An atlas of the Galactic plane (-4.7d < b < 4.7d), along with the molecular clouds in Orion, ρ Oph, and Taurus-Auriga, has been produced at 60 and 100 μm from IRAS data. The atlas consists of resolution-enhanced co-added images with 1'-2' resolution and co-added images at the native IRAS resolution. The IRAS Galaxy Atlas, together with the Dominion Radio Astrophysical Observatory H I line/21 cm continuum and FCRAO CO (1-0) Galactic plane surveys, which both have similar (~1') resolution to the IRAS atlas, provides a powerful tool for studying the interstellar medium, star formation, and large-scale structure in our Galaxy. This paper documents the production and characteristics of the atlas.
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