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Rethinking the N(H2)/I(CO) conversion factor

Monthly notices of the Royal Astronomical Society, 2007-08, Vol.379 (2), p.674-688

Wall, W. F.

2007

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Comparison of 13CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions – II. The simulations: testing the method

Monthly notices of the Royal Astronomical Society, 2007-05, Vol.377 (2), p.545-555

Wall, W. F.

2007

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Submillimeter to centimeter excess emission from the Magellanic Clouds II. On the nature of the excess

Astronomy and astrophysics (Berlin), 2010-11, Vol.523, p.A20

2010

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Comparison of 13CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - I. Motivation and modelling

Monthly notices of the Royal Astronomical Society, 2007-02, Vol.375 (1), p.278-300

Wall, W. F.

2007

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Submillimeter to centimeter excess emission from the Magellanic Clouds I. Global spectral energy distribution

Astronomy and astrophysics (Berlin), 2010-09, Vol.519, p.A67

2010

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Spatially Resolved Dust, Gas, and Star Formation in the Dwarf Magellanic Irregular NGC 4449

The Astrophysical journal, 2018-01, Vol.852 (2), p.106

2018

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Continuum observations of M 51 and M 83 at 1.1 mm with AzTEC

Monthly notices of the Royal Astronomical Society, 2016-06, Vol.459 (2), p.1440-1467

2016

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Molecular gas and dust in the highly magnified z ~ 2.8 galaxy behind the Bullet Cluster

Astronomy and astrophysics (Berlin), 2012-07, Vol.543, p.A62

2012

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Submillimeter to centimeter excess emission from the Magellanic Clouds

Astronomy and astrophysics (Berlin), 2010-11, Vol.523

2010

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Submillimeter to centimeter excess emission from the Magellanic Clouds

Astronomy and astrophysics (Berlin), 2010-09, Vol.519

2010

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Kiloparsec-scale molecular gas excitation in spiral galaxies

The Astrophysical journal, 1993-09, Vol.414 (1), p.98-111

1993

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The N(H2)/I(CO) Conversion Factor: A Treatment that Includes Radiative Transfer

Revista mexicana de astronomía y astrofísica, 2006-04, Vol.42 (1), p.117-126

Wall, W. F.

2006

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Molecular gas excitation in NGC 253

The Astrophysical journal, 1991-10, Vol.380 (2), p.384-391

1991

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Rethinking the N(H2)/I(CO) conversion factor

Monthly notices of the Royal Astronomical Society, 2007-08, Vol.379 (2), p.674-688

Wall, W. F.

2007

Volltextzugriff (PDF)

Comparison of 13 CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - III. Systematic effects and scientific implications

Monthly notices of the Royal Astronomical Society, 2007-05, Vol.377 (2), p.556-570, Article 556

Wall, W. F.

2007

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Comparison of super(13)CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - III. Systematic effects and scientific implications

Monthly notices of the Royal Astronomical Society, 2007-05, Vol.377 (2), p.556-570

Wall, W F

2007

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Comparison of 13CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - III. Systematic effects and scientific implications

Monthly notices of the Royal Astronomical Society, 2007-05, Vol.377 (2), p.556-570

Wall, W. F.

2007

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Comparison of 13CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - II. The simulations: testing the method

Monthly notices of the Royal Astronomical Society, 2007-05, Vol.377 (2), p.545-555

Wall, W. F.

2007

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Comparison of 13 CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - II. The simulations: testing the method

Monthly notices of the Royal Astronomical Society, 2007-05, Vol.377 (2), p.545-555, Article 545

Wall, W. F.

2007

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Comparison of super(13)CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - II. The simulations: testing the method

Monthly notices of the Royal Astronomical Society, 2007-05, Vol.377 (2), p.545-555

Wall, W F

2007

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Early Science with the Large Millimeter Telescope: discovery of the 12 CO(1–0) emission line in the ring galaxy VIIZw466

Monthly notices of the Royal Astronomical Society, 2017-04, Vol.466 (1), p.574-580

2017

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Early Science with the Large Millimeter Telescope: discovery of the 12CO(1-0) emission line in the ring galaxy VIIZw466

Monthly notices of the Royal Astronomical Society, 2017-04, Vol.466 (1), p.574-574

2017

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Extended CO(7-6) emission from warm gas in Orion

The Astrophysical journal, 1993-06, Vol.410 (1), p.179-187

1993

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Molecular gas and dust in the highly magnified z similar to 2.8 galaxy behind the Bullet Cluster

Astronomy and astrophysics (Berlin), 2012-07, Vol.543, p.Article Number: A62 (pp. 1

2012

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Rethinking the N(H2)/I(CO) conversion factor

Comparison of 13CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions – II. The simulations: testing the method

Submillimeter to centimeter excess emission from the Magellanic Clouds II. On the nature of the excess

Comparison of 13CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - I. Motivation and modelling

Submillimeter to centimeter excess emission from the Magellanic Clouds I. Global spectral energy distribution

Spatially Resolved Dust, Gas, and Star Formation in the Dwarf Magellanic Irregular NGC 4449

Continuum observations of M 51 and M 83 at 1.1 mm with AzTEC

Molecular gas and dust in the highly magnified z ~ 2.8 galaxy behind the Bullet Cluster

Submillimeter to centimeter excess emission from the Magellanic Clouds

Submillimeter to centimeter excess emission from the Magellanic Clouds

Kiloparsec-scale molecular gas excitation in spiral galaxies

The N(H2)/I(CO) Conversion Factor: A Treatment that Includes Radiative Transfer

Molecular gas excitation in NGC 253

Rethinking the N(H2)/I(CO) conversion factor

Comparison of 13 CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - III. Systematic effects and scientific implications

Comparison of super(13)CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - III. Systematic effects and scientific implications

Comparison of 13CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - III. Systematic effects and scientific implications

Comparison of 13CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - II. The simulations: testing the method

Comparison of 13 CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - II. The simulations: testing the method

Comparison of super(13)CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - II. The simulations: testing the method

Spatially Resolved Dust, Gas, and Star Formation in the Dwarf Magellanic Irregular NGC 4449 Based on observations obtained with the Large Millimeter Telescope Alfonso Serrano-a binational collaboration between INAOE (Mexico) and the University of Massachusetts-Amherst (USA)

Early Science with the Large Millimeter Telescope: discovery of the 12 CO(1–0) emission line in the ring galaxy VIIZw466

Early Science with the Large Millimeter Telescope: discovery of the 12CO(1-0) emission line in the ring galaxy VIIZw466

Extended CO(7-6) emission from warm gas in Orion

Molecular gas and dust in the highly magnified z similar to 2.8 galaxy behind the Bullet Cluster

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