Laboratory Measurement of CH317OH Transitions in the Frequency Range from 216 to 264 GHz for Astronomical Application
Methanol is one of the most abundant complex organic molecules in interstellar environments. Molecular lines of its rare isotopologues ^12 CH _3 ^17 OH and ^12 CH _3 ^18 OH therefore play a crucial role in examining the column density of ^12 CH _3 ^16 OH, which serves as a reference for organic mole...
Saved in:
Main Authors: | Akemi Tamanai, Takahiro Oyama, Yoshimasa Watanabe, Takeshi Sakai, Riouhei Nakatani, Shaoshan Zeng, Isabelle Kleiner, Nami Sakai |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/ad9b16 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Laboratory Rotational Spectroscopy Leads to the First Interstellar Detection of Singly Deuterated Methyl Mercaptan (CH2DSH)
by: Hayley A. Bunn, et al.
Published: (2025-01-01) -
CH3OH Thermal Lines Traces 6.7 GHz CH3OH Maser Variation of High-mass Protostar G353.273+0.641
by: Shi-Min Song, et al.
Published: (2025-01-01) -
Molecular Distributions and Abundances in the Binary-shaped Outflow of V Hya
by: Mark A. Siebert, et al.
Published: (2025-01-01) -
Design and Implementation of Xinjiang Astronomical Observatory Astronomical Data Transmission Visualization System
by: Xinchen Ye, et al.
Published: (2019-01-01) -
Clinics in diagnostic imaging (216)
by: Vishal Gaikwad, et al.
Published: (2023-05-01)