Tracing Interstellar Heating: An ALCHEMI Measurement of the HCN Isomers in NGC 253
Artikel i vetenskaplig tidskrift, 2022

We analyze HCN and HNC emission in the nearby starburst galaxy NGC 253 to investigate its effectiveness in tracing heating processes associated with star formation. This study uses multiple HCN and HNC rotational transitions observed using the Atacama Large Millimeter/submillimeter Array via the ALCHEMI Large Program. To understand the conditions and associated heating mechanisms within NGC 253's dense gas, we employ Bayesian nested sampling techniques applied to chemical and radiative transfer models, which are constrained using our HCN and HNC measurements. We find that the volume density n H 2 and cosmic-ray ionization rate (CRIR) ζ are enhanced by about an order of magnitude in the galaxy’s central regions as compared to those further from the nucleus. In NGC 253's central giant molecular clouds (GMCs), where observed HCN/HNC abundance ratios are the lowest, n ∼ 105.5 cm−3 and ζ ∼ 10−12 s−1 (greater than 104 times the average Galactic rate). We find a positive correlation in the association of both density and CRIR with the number of star formation-related heating sources (supernova remnants, H ii regions, and super hot cores) located in each GMC, as well as a correlation between CRIRs and supernova rates. Additionally, we see an anticorrelation between the HCN/HNC ratio and CRIR, indicating that this ratio will be lower in regions where ζ is higher. Though previous studies suggested HCN and HNC may reveal strong mechanical heating processes in NGC 253's CMZ, we find cosmic-ray heating dominates the heating budget, and mechanical heating does not play a significant role in the HCN and HNC chemistry.

Författare

E. Behrens

University of Virginia

J. G. Mangum

National Radio Astronomy Observatory

Jonathan Holdship

Universiteit Leiden

University College London (UCL)

Serena Viti

University College London (UCL)

Universiteit Leiden

N. Harada

The Graduate University for Advanced Studies (SOKENDAI)

National Astronomical Observatory of Japan

S. Martin

European Southern Observatory Santiago

Atacama Large Millimeter-submillimeter Array (ALMA)

K. Sakamoto

Academia Sinica

Sebastien Muller

Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium

Kunihiko Tanaka

Keio University

Kouichiro Nakanishi

The Graduate University for Advanced Studies (SOKENDAI)

National Astronomical Observatory of Japan

R. Herrero-Illana

European Southern Observatory Santiago

Institut de Ciències de l'Espai (ICE) - CSIC

Y. Yoshimura

University of Tokyo

Rebeca Aladro

Max-Planck-Gesellschaft

L. Colzi

Centro de Astrobiologia (CAB)

K.L. Emig

National Radio Astronomy Observatory

C. Henkel

Max-Planck-Gesellschaft

King Abdulaziz University

K. Y. Huang

Universiteit Leiden

Pedro Humire

Max-Planck-Gesellschaft

D. S. Meier

National Radio Astronomy Observatory Socorro

New Mexico Institute of Mining and Technology

Víctor M. Rivilla

Centro de Astrobiologia (CAB)

P. van der Werf

Universiteit Leiden

Astrophysical Journal

0004-637X (ISSN) 1538-4357 (eISSN)

Vol. 939 2 119

Ämneskategorier

Energiteknik

Astronomi, astrofysik och kosmologi

Atom- och molekylfysik och optik

DOI

10.3847/1538-4357/ac91ce

Mer information

Senast uppdaterat

2022-12-01