Potential lines of formic acid for its detection in cosmic objects

被引:0
作者
Mohit K. Sharma
Suresh Chandra
机构
[1] Sunder Deep Group of Institutions,Physics Department
[2] Amity University,Amity Centre for Astronomy & Astrophysics, Amity Institute of Applied Sciences
来源
Journal of Astrophysics and Astronomy | 2021年 / 42卷
关键词
ISM: molecules; HCOOH; Einstein ; -coefficients; radiative transfer; astrobiology;
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摘要
Being precursor for amino acids (constituents of life), the simplest carboxylic acid, formic acid (HCOOH) has great importance in astrobiology. It has two rotameric isomers: trans-HCOOH and cis-HCOOH, each of which, due to the delocalization of π\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\pi$$\end{document}-electrons over the heavy atom chain, lies in a plane. The electric dipole moment of each isomer has a and b components and energy levels for both components are common. It is, therefore, more scientific to consider both components of electric dipole moment together. The stronger isomer trans-HCOOH has been detected in several cosmic objects through its 16 a-type transitions, because its μb\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\mu _b$$\end{document} is very small as compared to μa\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\mu _a$$\end{document}. The cis-HCOOH has been detected in Orion Bar through 12a and b types of transitions.
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