2014A&A...563A.127M


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.06CEST23:44:14

2014A&A...563A.127M - Astronomy and Astrophysics, volume 563A, 127-127 (2014/3-1)

Ionization toward the high-mass star-forming region NGC 6334 I.

MORALES ORTIZ J.L., CECCARELLI C., LIS D.C., OLMI L., PLUME R. and SCHILKE P.

Abstract (from CDS):

Ionization plays a central role in the gas-phase chemistry of molecular clouds. Since ions are coupled with magnetic fields, which can in turn counteract gravitational collapse, it is of paramount importance to measure their abundance in star-forming regions. We use spectral line observations of the high-mass star-forming region NGC 6334I to derive the abundance of two of the most abundant molecular ions, HCO+ and N2H+, and consequently, the cosmic ray ionization rate. In addition, the line profiles provide information about the kinematics of this region. We present high-resolution spectral line observations conducted with the HIFI instrument on board the Herschel Space Observatory of the rotational transitions with Jup≥5 of the molecular species C17O, C18O, HCO+, H13CO+, and N2H+. The HCO+ and N2H+ line profiles display a redshifted asymmetry consistent with a region of expanding gas. We identify two emission components in the spectra, each with a different excitation, associated with the envelope of NGC 6334I. The physical parameters obtained for the envelope are in agreement with previous models of the radial structure of NGC 6334I based on submillimeter continuum observations. Based on our new Herschel/HIFI observations, combined with the predictions from a chemical model, we derive a cosmic ray ionization rate that is an order of magnitude higher than the canonical value of 10–17s–1. We find evidence of an expansion of the envelope surrounding the hot core of NGC 6334I, which is mainly driven by thermal pressure from the hot ionized gas in the region. The ionization rate seems to be dominated by cosmic rays originating from outside the source, although X-ray emission from the NGC 6334I core could contribute to the ionization in the inner part of the envelope.

Abstract Copyright:

Journal keyword(s): stars: formation - ISM: clouds - ISM: molecules - cosmic rays - ISM: abundances

Simbad objects: 8

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Number of rows : 8

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 NGC 6334 HII 17 20 51 -36 06.9           ~ 585 0
2 [HBM2006b] I-SMA4 mm 17 20 53.099 -35 47 03.32           ~ 9 0
3 [BHC2016] MM2 mm 17 20 53.188 -35 46 59.32           ~ 25 0
4 NAME NGC 6334-I Cl* 17 20 53.35 -35 47 01.5           ~ 269 0
5 [BHC2016] MM1 mm 17 20 53.415 -35 46 57.88           ~ 47 0
6 NAME NGC 6334F (C) HII 17 20 53.45 -35 47 02.6           ~ 206 1
7 NAME Gal Center reg 17 45 40.04 -29 00 28.1           ~ 11533 0
8 [HG83] IRS-I-1E IR 21 20 37.06 -35 31 20.2           ~ 6 0

    Equat.    Gal    SGal    Ecl

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2020.07.06-23:44:14

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