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Molecular clouds in the Milky Way
M Heyer, TM Dame - Annual Review of Astronomy and …, 2015 - annualreviews.org
In the past twenty years, the reconnaissance of 12CO and 13CO emission in the Milky Way
by single-dish millimeter-wave telescopes has expanded our view and understanding of …
by single-dish millimeter-wave telescopes has expanded our view and understanding of …
[HTML][HTML] A new component of the interstellar matter-Small grains and large aromatic molecules
JL Puget, A Leger - IN: Annual review of astronomy and …, 1989 - adsabs.harvard.edu
Dust models have been constructed to account for the interstellar extinction curve.
Unfortunately, when emission data became available, they were in conflict with the …
Unfortunately, when emission data became available, they were in conflict with the …
The Milky Way in Molecular Clouds: A New Complete COSurvey
TM Dame, D Hartmann, P Thaddeus - The Astrophysical Journal, 2001 - iopscience.iop.org
New large-scale CO surveys of the first and second Galactic quadrants and the nearby
molecular cloud complexes in Orion and Taurus, obtained with the CfA 1.2 m telescope …
molecular cloud complexes in Orion and Taurus, obtained with the CfA 1.2 m telescope …
Infrared emission from interstellar dust. II. The diffuse interstellar medium
A Li, BT Draine - The Astrophysical Journal, 2001 - iopscience.iop.org
We present a quantitative model for the infrared emission from dust in the diffuse interstellar
medium. The model consists of a mixture of amorphous silicate grains and carbonaceous …
medium. The model consists of a mixture of amorphous silicate grains and carbonaceous …
[HTML][HTML] Collisional charging of interstellar grains
BT Draine, B Sutin - Astrophysical Journal, Part 1 (ISSN 0004 …, 1987 - adsabs.harvard.edu
grain charge is small. The probability distribution for the grain charge is obtained for the
case of pure collisional charging (ie, photoelectric emission due to background ultraviolet is …
case of pure collisional charging (ie, photoelectric emission due to background ultraviolet is …
PHANGS–JWST First Results: Tracing the Diffuse Interstellar Medium with JWST Imaging of Polycyclic Aromatic Hydrocarbon Emission in Nearby Galaxies
KM Sandstrom, EW Koch, AK Leroy… - The Astrophysical …, 2023 - iopscience.iop.org
JWST observations of polycyclic aromatic hydrocarbon (PAH) emission provide some of the
deepest and highest resolution views of the cold interstellar medium (ISM) in nearby …
deepest and highest resolution views of the cold interstellar medium (ISM) in nearby …
[HTML][HTML] Are polycyclic aromatic hydrocarbons the carriers of the diffuse interstellar bands in the visible?
A Léger, L d'Hendecourt - … (ISSN 0004-6361), vol. 146, no. 1 …, 1985 - adsabs.harvard.edu
Are polycyclic aromatic hydrocarbons the carriers of the diffuse interstellar ba ADS Classic is
now deprecated. It will be completely retired in October 2019. This page will automatically …
now deprecated. It will be completely retired in October 2019. This page will automatically …
[HTML][HTML] Diffuse infrared emission from the galaxy. I-Solar neighborhood
F Boulanger, M Perault - … Journal, Part 1 (ISSN 0004-637X), vol …, 1988 - adsabs.harvard.edu
Diffuse infrared emission from the galaxy. I - Solar neighborhood ADS Classic is now
deprecated. It will be completely retired in October 2019. This page will automatically redirect to …
deprecated. It will be completely retired in October 2019. This page will automatically redirect to …
[HTML][HTML] Star formation and dust extinction in disk galaxies. Comparison between the UV non-ionizing and the FIR emissions
V Buat, C Xu - Astronomy and Astrophysics, v. 306, p. 61, 1996 - adsabs.harvard.edu
We have used a radiation transfer model to estimate the extinction in galactic disks
considering their ultraviolet, optical and infrared emission and applied this model to a …
considering their ultraviolet, optical and infrared emission and applied this model to a …
Models for infrared emission from IRAS galaxies
M Rowan-Robinson, J Crawford - Monthly Notices of the Royal …, 1989 - academic.oup.com
Abstract The far-infrared (10–100 μ m) spectra of galaxies detected in all four wavelength
bands by IRAS are modelled in terms of three components: a cool 'disc'component; a …
bands by IRAS are modelled in terms of three components: a cool 'disc'component; a …