Differences in chemical evolution between isolated and embedded prestellar cores
Author:
Affiliation:
1. School of Physics and Astronomy, Cardiff University , Queen’s Buildings, The Parade, Cardiff CF24 3AA, UK
2. Center for Theoretical Astrophysics, Los Alamos National Laboratory , Los Alamos, NM 87545, USA
Abstract
Funder
Science and Technology Facilities Council
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stac3444/47267076/stac3444.pdf
Reference36 articles.
1. Molecular Evolution in Collapsing Prestellar Cores. III. Contraction of a Bonnor‐Ebert Sphere
2. An ALMA study of hub-filament systems – I. On the clump mass concentration within the most massive cores
3. TIMESCALES FOR LOW-MASS STAR FORMATION IN EXTRAGALACTIC ENVIRONMENTS: IMPLICATIONS FOR THE STELLAR INITIAL MASS FUNCTION
4. Cold Dark Clouds: The Initial Conditions for Star Formation
5. Smoothed particle hydrodynamics simulations of expanding H II regions
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1. Insights into the first and second hydrostatic core stages from numerical simulations;Frontiers in Astronomy and Space Sciences;2023-12-07
2. Non-Equilibrium Abundances Treated Holistically (NEATH): the molecular composition of star-forming clouds;Monthly Notices of the Royal Astronomical Society;2023-07-26
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