Spectroscopy of bright Algol-type semi-detached close binary system HU Tauri (HR 1471)
M. Parthasarathy
TL;DR
This paper presents spectroscopic analysis of the Algol-type binary HU Tauri, confirming the secondary star's H-alpha emission using high-resolution spectra, contributing to understanding its spectral characteristics.
Contribution
First spectroscopic detection of the secondary's H-alpha line in HU Tauri, verified with high-resolution spectra from McDonald Observatory.
Findings
Detection of H-alpha line of the secondary star.
Confirmation of spectral features with high-resolution data.
Provides detailed spectroscopic data for HU Tauri.
Abstract
Spectroscopic results of HU Tauri that I presented in my Ph.D thesis (Parthasarathy 1979) are published in this paper. The H-alpha line of the secondary is detected. The detection of H-alpha line of the secondary is confirmed based on the high resolution Coude Reticon spectra obtained with the 2.1-m telescope of the McDonald observatory.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.