Detection of the HC3NH+ and HCNH+ ions in the L1544 pre-stellar core-Reference-Cited by-同舟云学术

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Detection of the HC3NH+ and HCNH+ ions in the L1544 pre-stellar core

Published:2017-06-03 Issue:3 Volume:470 Page:3194-3205
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Quénard D.¹²³,Vastel C.²³,Ceccarelli C.⁴,Hily-Blant P.⁴,Lefloch B.⁴,Bachiller R.⁵

Affiliation:

1. School of Physics and Astronomy, Queen Mary University of London, Mile End Road, London E1 4NS, UK

2. Université de Toulouse, UPS-OMP, IRAP, Toulouse, France

3. CNRS, IRAP, 9 Av. Colonel Roche, BP 44346, F-31028 Toulouse Cedex 4, France

4. Univ. Grenoble Alpes, CNRS, IPAG, F-38000 Grenoble, France

5. Observatorio Astronómico Nacional (OAN, IGN), Calle Alfonso XII, 3, E-28014 Madrid, Spain

Funder

CNRS

STFC

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/470/3/3194/18548190/stx1373.pdf

Reference52 articles.

1. Chemistry of Dark Clouds: Databases, Networks, and Models

2. Probing non-polar interstellar molecules through their protonated form: Detection of protonated cyanogen (NCCNH+)

3. Search for HC3NH(+) - The upper limit of the column density in TMC-1

4. Molecular Ions in L1544. I. Kinematics

5. Molecular Ions in L1544. II. The Ionization Degree

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1. Hyperfine-resolved rotational spectroscopy of HCNH+;The Journal of Chemical Physics;2024-02-15

2. HCNH⁺ abundance in cold dense clouds based on the first hyperfine resolved rate coefficients;Astronomy & Astrophysics;2024-01

3. O Corona, where art thou? eROSITA’s view of UV-optical-IR variability-selected massive black holes in low-mass galaxies;Astronomy & Astrophysics;2024-01

4. Protonated hydrogen cyanide as a tracer of pristine molecular gas;Astronomy & Astrophysics;2023-11

5. Similar levels of deuteration in the pre-stellar core L1544 and the protostellar core HH211;Astronomy & Astrophysics;2023-08

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