Organic molecules in the interstellar medium, comets, and meteorites: a voyage from dark clouds to the early Earth
P Ehrenfreund, SB Charnley - Annual Review of Astronomy and …, 2000 - annualreviews.org
▪ Abstract Our understanding of the evolution of organic molecules, and their voyage from
molecular clouds to the early solar system and Earth, has changed dramatically …
molecular clouds to the early solar system and Earth, has changed dramatically …
Reaction networks for interstellar chemical modelling: improvements and challenges
We survey the current situation regarding chemical modelling of the synthesis of molecules
in the interstellar medium. The present state of knowledge concerning the rate coefficients …
in the interstellar medium. The present state of knowledge concerning the rate coefficients …
The UMIST database for astrochemistry 1995
TJ Millar, PRA Farquhar, K Willacy - Astronomy and Astrophysics …, 1997 - aas.aanda.org
We report the release of a new version of the UMIST database for astrochemistry. The
database contains the rate coefficients of 3864 gas-phase reactions important in interstellar …
database contains the rate coefficients of 3864 gas-phase reactions important in interstellar …
Carbon stars
G Wallerstein, GR Knapp - Annual Review of Astronomy and …, 1998 - annualreviews.org
▪ Abstract Absolute magnitudes are estimated for carbon stars of various subtypes in the
Hipparcos catalogue and as found in the Magellanic Clouds. Stellar radii fall within the limits …
Hipparcos catalogue and as found in the Magellanic Clouds. Stellar radii fall within the limits …
[HTML][HTML] Detection of MgCN in IRC+ 10216: A new metal-bearing free radical
LM Ziurys, AJ Apponi, M Guélin… - … 637X), vol. 445, no. 1, p …, 1995 - adsabs.harvard.edu
Detection of MgCN in IRC + 10216: A new metal-bearing free radical 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 …
A chemical study of the inner winds of asymptotic giant branch stars
I Cherchneff - Astronomy & Astrophysics, 2006 - aanda.org
Aims. We investigate the non-equilibrium chemistry of the inner winds of AGB stars for
different stages of stellar evolution, choosing a standard AGB stellar model and changing …
different stages of stellar evolution, choosing a standard AGB stellar model and changing …
Large molecules in the envelope surrounding IRC+ 10216
A new chemical model of the circumstellar envelope surrounding the carbon-rich star IRC+
10216 is developed that includes carbon-containing molecules with up to 23 carbon atoms …
10216 is developed that includes carbon-containing molecules with up to 23 carbon atoms …
Neutral–neutral reactions at the temperatures of interstellar clouds Rate coefficients for reactions of C 2 H radicals with O 2, C 2 H 2, C 2 H 4 and C 3 H 6 down to 15 K
D Chastaing, PL James, IR Sims, IWM Smith - Faraday Discussions, 1998 - pubs.rsc.org
A CRESU (Cine′ tique de Re′ action en Ecoulement Supersonique Uniforme) apparatus
has been used to measure rate constants for the reactions of the ethynyl radical (C2H) with …
has been used to measure rate constants for the reactions of the ethynyl radical (C2H) with …
Circumstellar and interstellar synthesis of organic molecules
A Tielens, SB Charnley - Origins of Life and Evolution of the Biosphere, 1997 - Springer
We review the formation and evolution of complex circumstellar and interstellar molecules. A
number of promising chemical routes are discussed which may lead to the formation of …
number of promising chemical routes are discussed which may lead to the formation of …
Far-infrared detection of C3 in Sagittarius B2 and IRC+ 10216
J Cernicharo, JR Goicoechea… - The Astrophysical …, 2000 - iopscience.iop.org
We report on the detection of nine lines of the ν 2 bending mode of triatomic carbon, C 3, in
the direction of Sagittarius B2. The R (4) and R (2) lines of C 3 have been also detected in …
the direction of Sagittarius B2. The R (4) and R (2) lines of C 3 have been also detected in …