User profiles for A. Tielens

AGGM Tielens

professor of Astrophysics, Astronomy Department, University of Maryland & Leiden …
Verified email at umd.edu
Cited by 77991

The molecular universe

A Tielens - Reviews of Modern Physics, 2013 - APS
Molecular absorption and emission bands dominate the visible, infrared, and submillimeter
spectra of most objects with associated gas. These observations reveal a surprisingly rich …

Interstellar polycyclic aromatic hydrocarbon molecules

AGGM Tielens - Annu. Rev. Astron. Astrophys., 2008 - annualreviews.org
Large polycyclic aromatic hydrocarbon (PAH) molecules carry the infrared (IR) emission
features that dominate the spectra of most galactic and extragalactic sources. This review …

[HTML][HTML] Interstellar polycyclic aromatic hydrocarbons-The infrared emission bands, the excitation/emission mechanism, and the astrophysical implications

LJ Allamandola, A Tielens… - … , vol. 71, Dec. 1989, p. 733 …, 1989 - adsabs.harvard.edu
… on a strong continuum which follows a 1/X law (Tielens and … assume that JR emission
originates in the neutral photodissociation regions (Tielens and Hollenbach 1985a, b) …

[BOOK][B] The physics and chemistry of the interstellar medium

AGGM Tielens - 2005 - books.google.com
This work provides a comprehensive overview of our theoretical and observational understanding
of the interstellar medium of galaxies. With emphasis on the microscopic physical and …

[HTML][HTML] Interstellar solid CO-Polar and nonpolar interstellar ices

A Tielens, AT Tokunaga, TR Geballe… - … Journal, Part 1 (ISSN …, 1991 - adsabs.harvard.edu
Observations of the solid-CO lines corresponding to particular protostars are compared with
respect to peak position and width and contrasted with the solid CO bands derived …

[HTML][HTML] Polycyclic aromatic hydrocarbons and the unidentified infrared emission bands-Auto exhaust along the Milky Way

LJ Allamandola, A Tielens… - … Part 2-Letters to the Editor …, 1985 - adsabs.harvard.edu
… LJ ALLAMANDOLA' AND AGGM TIELENS … of about 20 (Allamandola, Tielens, and
Barker 1984). Jf all of … dominated by the 1-0 transition (Allamandola, Tielens, and …

Interstellar ice: the infrared space observatory legacy

…, DCB Whittet, ACA Boogert, A Tielens - The astrophysical …, 2004 - iopscience.iop.org
We present 2.5–30 μ m spectra from the Short-Wavelength Spectrometer of the Infrared
Space Observatory for a total of 23 sources. The sources include embedded young stellar …

[HTML][HTML] The photoelectric heating mechanism for very small graphitic grains and polycyclic aromatic hydrocarbons

ELO Bakes, A Tielens - … Journal, Part 1 (ISSN 0004-637X), vol …, 1994 - adsabs.harvard.edu
We have theoretically modeled the gas heating associated with the photoelectric ejection of
electrons from a size distribution of interstellar carbon grains which extends into the …

[HTML][HTML] Neutral atomic phases of the interstellar medium in the galaxy

…, CF McKee, D Hollenbach, A Tielens - The Astrophysical …, 2003 - iopscience.iop.org
Much of the interstellar medium in disk galaxies is in the form of neutral atomic hydrogen, H I.
This gas can be in thermal equilibrium at relatively low temperatures, T≲ 300 K (the cold …

[HTML][HTML] Grain shattering in shocks: The interstellar grain size distribution

AP Jones, A Tielens… - Astrophysical Journal v …, 1996 - adsabs.harvard.edu
We have studied the effects of shattering in grain-grain collisions. Based upon extensive
numerical simulation of surface explosions and impacts, an analytical model has been …