Identification of beryllium hydride isotopomer lines in sunspot umbral spectra

Author:

Shanmugavel R.1,Bagare S.P.2,Rajamanickam N.1,Kumar Balachandra3

Affiliation:

1. Physics Research Centre, V.H.N.S.N College, Virudhunagar, India

2. Indian Institute of Astrophysics, Kodaikanal & Bangalore, India

3. Kamaraj College of Engineering and Technology, Virudhunagar, India

Abstract

A high resolution spectrum of FTS sunspot umbra of NSO/Kitt Peak was used to conduct a search for the molecular absorption lines due to BeH, BeD and BeT isotopomers. Analysis led to estimates of identification of the molecular lines of bands A - X (0,0), (1,1) and (2,2) for BeH, A - X (0,0), (1,1), (2,2) and (3,3) for BeD and of A - X (0,0), (1,1) and (2,2) for BeT. Among the identified lines, those which are well resolved were selected for measurements to calculate equivalent widths. The values of effective rotational temperature T were estimated for bands A - X(1,1) and (2,2) of BeH, A - X(1,1) of BeD and A - X(2,2) of BeT to be 4228K, 4057K, 3941K and 3243K respectively.

Publisher

National Library of Serbia

Subject

Astronomy and Astrophysics

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4. Molecular opacities of the transitions for the lowest four singlet states of BeH+;Journal of Quantitative Spectroscopy and Radiative Transfer;2018-02

5. Molecular Constants of BeH X 2Σ+ Beryllium Hydride;Molecular Constants Mostly from Microwave, Molecular Beam, and Sub-Doppler Laser Spectroscopy;2017

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