A spectroscopic survey of Orion KL between 41.5 and 50 GHz
Author:
Funder
MICINN
MINECO
ERC
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/201629936/pdf
Reference55 articles.
1. Detection of Methyl Alcohol in Orion at a Wavelength of ~1 Centimeter
2. Line Imaging of Orion KL at 865 μm with the Submillimeter Array
3. Molecular abundances in OMC-1 - The chemical composition of interstellar molecular clouds and the influence of massive star formation
4. On the Interpretation of Radio Recombination Line Observations
5. CH3OCH3in Orion-KL: a striking similarity with HCOOCH3
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1. Large-scale Mapping Observations of DCN and DCO+ toward Orion KL;The Astrophysical Journal;2024-02-22
2. The First Ka-band (26.1–35 GHz) Blind Line Survey toward Orion KL;The Astrophysical Journal Supplement Series;2024-02-12
3. The Mid-infrared Molecular Inventory toward Orion IRc2;The Astrophysical Journal;2023-03-01
4. A Q-band Line Survey toward Orion KL Using the Tianma Radio Telescope;The Astrophysical Journal Supplement Series;2022-11-01
5. Anatomy of Orion Molecular Clouds—The Astrochemistry Perspective/Approach;Frontiers in Astronomy and Space Sciences;2021-10-15
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