One-dimensional and time-dependent modelling of complex organic molecules in protostars

Astronomy and Astrophysics, vol. 708, pp. A92

Abstract

Complex organic molecules (COMs), the building blocks of life, have been extensively detected under various physical conditions, from quiescent clouds to star-forming regions. They therefore serve as excellent tracers of the local physical and chemical properties of these environments. Proper models that are capable of grasping the formation and destruction of COMs are crucial to understanding observations. However, given that distinct COMs can be detected from different locations and at varying times, we improved UCLCHEM – a gas-grain chemical code – to a 1D, time-dependent model tailored to protostars. In this update, we examine two stages of a protostar, the prestellar and heating stages, incorporating a simple radiative mechanism for both the internal and external radiation fields of the cloud. This approach relies on the key assumption that the dust and gas temperatures are completely coupled. Ultimately, we implemented an updated version of our model to interpret observations obtained through both single-dish and interferometry under varying conditions, including a SgrB2(N1) hot core, massive Galactic clumps, and a hot core in Orion. We show that our model can reproduce these observations well. We highlight that some COMs are positioned at a higher temperature in the envelope, and others at a lower temperature, which could potentially leading to misinterpretations when using a single-point model. In the case of SgrB2(N1), the best model indicates that the cosmic-ray ionisation rate significantly exceeds the value typically used for the standard interstellar medium. Our model is as an efficient computational tool that will be particularly useful for gaining better insights into COM observations.

Authors 8

1. Le Ngoc Tram Aachen Leiden Observatory

   Leiden University · Leiden Observatory

   Affiliation as printed

   Leiden Observatory, Leiden University

2. S. Viti Aachen Leiden Observatory

   Leiden University · University of Bonn · Leiden Observatory · University College London

   Affiliation as printed

   Department of Physics and Astronomy, University College London

   Leiden Observatory, Leiden University

   Transdisciplinary Research Area (TRA) ‘Matter’/Argelander-Institut für Astronomie, University of Bonn

3. K. M. Dutkowska Aachen Leiden Observatory

   Leiden University · Leiden Observatory

   Affiliation as printed

   Leiden Observatory, Leiden University

4. Gijs Vermariën Aachen Leiden Observatory

   Leiden University · SURF · Leiden Observatory

   Affiliation as printed

   Leiden Observatory, Leiden University

   SURF

5. Tobias M. Dijkhuis Aachen Leiden Observatory

   Leiden University · Radboud University Nijmegen · Leiden Observatory

   Affiliation as printed

   Institute for Molecules and Materials, Radboud University

   Leiden Institute of Chemistry, Leiden University

   Leiden Observatory, Leiden University

6. A. Coutens

   Centre National de la Recherche Scientifique · Institut de Recherche en Astrophysique et Planétologie · Université de Toulouse

   Affiliation as printed

   Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse, CNRS, CNES

7. T. Csengeri

   Centre National de la Recherche Scientifique · Université de Bordeaux · Laboratoire d'Astrophysique de Bordeaux

   Affiliation as printed

   Laboratoire d’astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire

8. Thiem Hoang

   Korea Astronomy and Space Science Institute · Korea University of Science and Technology

   Affiliation as printed

   Korea Astronomy and Space Science Institute

   Korea University of Science and Technology