3D modelling of HCO+ and its isotopologues in the low-mass proto-star IRAS16293−2422-Reference-Cited by-同舟云学术

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3D modelling of HCO+ and its isotopologues in the low-mass proto-star IRAS16293−2422

Published:2018-04-21 Issue:4 Volume:477 Page:5312-5326
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Quénard D¹²,Bottinelli S¹,Caux E¹,Wakelam V³

Affiliation:

1. IRAP, Université de Toulouse, CNRS, UPS, CNES, F-31028 Toulouse, France

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

3. Laboratoire d’astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, F-33615 Pessac, France

Funder

Science and Technology Facilities Council

European Research Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/477/4/5312/24865120/sty1004.pdf

Reference93 articles.

1. Molecular Evolution and Star Formation: From Prestellar Cores to Protostellar Cores

2. Pushing the Envelope: The Impact of an Outflow at the Earliest Stages of Star Formation

3. The Evolution of Outflow‐Envelope Interactions in Low‐Mass Protostars

4. Shock Chemistry in the Young Bipolar Outflow L1157

5. Magnetic braking, ambipolar diffusion, and the formation of cloud cores and protostars. 1: Axisymmetric solutions

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

2. Evidence for a Cosmic-Ray Gradient in the IM Lup Protoplanetary Disk;The Astrophysical Journal;2021-05-01

3. Ingredients for solar-like systems: protostar IRAS 16293-2422 B versus comet 67P/Churyumov–Gerasimenko;Monthly Notices of the Royal Astronomical Society;2019-09-02

4. The ALMA-PILS survey: gas dynamics in IRAS 16293−2422 and the connection between its two protostars;Astronomy & Astrophysics;2019-06

5. New constraints on the initial parameters of low-mass star formation from chemical modeling;Monthly Notices of the Royal Astronomical Society;2019-05-04

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