Observations of warm carbon chain chemistry in NGC 3576

M. Saul; N. F H Tothill; C. R. Purcell

doi:10.1088/0004-637X/798/1/36

Observations of warm carbon chain chemistry in NGC 3576

M. Saul^*, N. F H Tothill, C. R. Purcell

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

2 Citations (Scopus)

Abstract

We report observations of warm carbon chain chemistry (WCCC) in NGC 3576, including high angular resolution imaging of an ionization source candidate and the first detection of C₅H in a massive star-forming region. In order to investigate the environment associated with birthline emergence, we ask how observed chemical conditions relate to Class 0/1 core differentiation: a systemic shift in peak position between species correlates with giant molecular cloud core gradients in turbulence and age. Emission in several molecular lines including HC₃N (11-10), NH₃ (1, 1), and C₅H supports the G291.3-0.7 ionization front - transitional pre-main-sequence core interaction regulating the WCCC environment.

Original language	English
Article number	36
Pages (from-to)	1-9
Number of pages	9
Journal	Astrophysical Journal
Volume	798
Issue number	1
DOIs	https://doi.org/10.1088/0004-637X/798/1/36
Publication status	Published - 1 Jan 2015
Externally published	Yes

Keywords

Astrochemistry
Evolution
H II regions
ISM: abundances
Stars: formation
Turbulence

Access to Document

10.1088/0004-637X/798/1/36

Link to publication in Scopus

Fingerprint Dive into the research topics of 'Observations of warm carbon chain chemistry in NGC 3576'. Together they form a unique fingerprint.

Cite this

@article{f00bbfddb8b74a30a3c4d79729e0b74b,

title = "Observations of warm carbon chain chemistry in NGC 3576",

abstract = "We report observations of warm carbon chain chemistry (WCCC) in NGC 3576, including high angular resolution imaging of an ionization source candidate and the first detection of C5H in a massive star-forming region. In order to investigate the environment associated with birthline emergence, we ask how observed chemical conditions relate to Class 0/1 core differentiation: a systemic shift in peak position between species correlates with giant molecular cloud core gradients in turbulence and age. Emission in several molecular lines including HC3N (11-10), NH3 (1, 1), and C5H supports the G291.3-0.7 ionization front - transitional pre-main-sequence core interaction regulating the WCCC environment.",

keywords = "Astrochemistry, Evolution, H II regions, ISM: abundances, Stars: formation, Turbulence",

author = "M. Saul and Tothill, {N. F H} and Purcell, {C. R.}",

year = "2015",

month = jan,

day = "1",

doi = "10.1088/0004-637X/798/1/36",

language = "English",

volume = "798",

pages = "1--9",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing",

number = "1",

}

TY - JOUR

T1 - Observations of warm carbon chain chemistry in NGC 3576

AU - Saul, M.

AU - Tothill, N. F H

AU - Purcell, C. R.

PY - 2015/1/1

Y1 - 2015/1/1

N2 - We report observations of warm carbon chain chemistry (WCCC) in NGC 3576, including high angular resolution imaging of an ionization source candidate and the first detection of C5H in a massive star-forming region. In order to investigate the environment associated with birthline emergence, we ask how observed chemical conditions relate to Class 0/1 core differentiation: a systemic shift in peak position between species correlates with giant molecular cloud core gradients in turbulence and age. Emission in several molecular lines including HC3N (11-10), NH3 (1, 1), and C5H supports the G291.3-0.7 ionization front - transitional pre-main-sequence core interaction regulating the WCCC environment.

AB - We report observations of warm carbon chain chemistry (WCCC) in NGC 3576, including high angular resolution imaging of an ionization source candidate and the first detection of C5H in a massive star-forming region. In order to investigate the environment associated with birthline emergence, we ask how observed chemical conditions relate to Class 0/1 core differentiation: a systemic shift in peak position between species correlates with giant molecular cloud core gradients in turbulence and age. Emission in several molecular lines including HC3N (11-10), NH3 (1, 1), and C5H supports the G291.3-0.7 ionization front - transitional pre-main-sequence core interaction regulating the WCCC environment.

KW - Astrochemistry

KW - Evolution

KW - H II regions

KW - ISM: abundances

KW - Stars: formation

KW - Turbulence

UR - http://www.scopus.com/inward/record.url?scp=84919468994&partnerID=8YFLogxK

U2 - 10.1088/0004-637X/798/1/36

DO - 10.1088/0004-637X/798/1/36

M3 - Article

AN - SCOPUS:84919468994

VL - 798

SP - 1

EP - 9

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 1

M1 - 36

ER -