2007A&A...467..179P


C.D.S. - SIMBAD4 rel 1.7 - 2019.10.18CEST07:00:35

2007A&A...467..179P - Astronomy and Astrophysics, volume 467, 179-186 (2007/5-3)

Depletion and low gas temperature in the L183 (=L134N) prestellar core: the N2H+-N2D+ tool.

PAGANI L., BACMANN A., CABRIT S. and VASTEL C.

Abstract (from CDS):

The study of pre-stellar cores (PSCs) suffers from a lack of undepleted species to trace the physical properties of the gas in their very dense inner parts. We carry out detailed modelling of N2H+ and N2D+ cuts across the L183 main core to evaluate the depletion of these species and their usefulness as a probe of physical conditions in PSCs. We have developed a non-LTE (NLTE) Monte-Carlo code treating the 1D radiative transfer of both N2H+ and N2D+, making use of recently published collisional coefficients with He between individual hyperfine levels. The code includes line overlap between hyperfine transitions. An extensive set of core models is calculated and compared with observations. Special attention is paid to the issue of source coupling to the antenna beam. The best-fitting models indicate that i) gas in the core center is very cold (7±1K) and thermalized with dust; ii) depletion of N2H+ does occur, starting at densities 5-7x105cm–3 and reaching a factor of 6+13–3 in abundance; iii) deuterium fractionation reaches ∼70% at the core center; and iv) the density profile is proportional to r–1 out to ∼4000 AU, and to r–2 beyond. Our NLTE code could be used to (re-)interpret recent and upcoming observations of N2H+ and N2D+ in many pre-stellar cores of interest, to obtain better temperature and abundance profiles.

Abstract Copyright:

Journal keyword(s): ISM: abundances - ISM: molecules - radiative transfer - ISM: structure - ISM: individual objects: L183 - line: formation

Simbad objects: 5

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Number of rows : 5

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2019
#notes
1 NAME [BM89] L1498 PoC 04 10 51.4 +25 09 58           ~ 187 0
2 LDN 1498 DNe 04 11.0 +24 58           ~ 241 0
3 LDN 1517 DNe 04 55 45 +30 33.0           ~ 93 0
4 LDN 134 MoC 15 53 36.3 -04 35 26           ~ 193 0
5 LDN 183 MoC 15 54 12.2 -02 49 42           ~ 674 1

    Equat.    Gal    SGal    Ecl

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2019.10.18-07:00:36

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