Modelling line emission of deuterated H3+ from prestellar cores

Astronomy and Astrophysics

Volumn 509, Issue 1, 2010, Pages

  Sipila O ^a   Hugo, E ^b   Harju, J ^a   Asvany, O ^b   Juvela, M ^a   Schlemmer, S ^b  

^a UNIVERSITY OF HELSINKI   (Finland)

^b UNIVERSITY OF COLOGNE   (Germany)

Author keywords

Abundances ISM; Clouds Radio lines; ISM; ISM Astrochemistry Radiative transfer ISM; Molecules

Indexed keywords

ASTRONOMY; CHEMICAL ELEMENTS; CLOUDS; DEUTERIUM; HIGH FREQUENCY TELECOMMUNICATION LINES; MOLECULES; RADIATIVE TRANSFER; RADIO WAVES; SPIN DYNAMICS;

ABUNDANCES - ISM; ASTROCHEMISTRY; CORE MODEL; DENSE CORE; DENSITY DISTRIBUTIONS; DETECTABILITY; EXCITATION MODELS; HEAVY ELEMENTS; INTERSTELLAR MOLECULAR CLOUDS; ISM - ISM; ISM-MOLECULES; ISOTOPIC SYSTEMS; ISOTOPOLOGUES; LINE EMISSIONS; LINE PROFILES; NUCLEAR SPINS; PHYSICAL CONDITIONS; PHYSICAL MODEL; POWER-LAW; PRESTELLAR CORES; RATE COEFFICIENTS; REACTION SCHEMES; ROTATIONAL LEVELS; ROTATIONAL LINES; SPECTROSCOPIC PROBES;

MODELS;

EID: 76349116501     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913350     Document Type: Article

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