THE ROTATION EFFECTS TO THE EVOLUTION OF THE B-EMISSION STARS: CASE STUDY HR 8520, HR 8402, AND HR 5941

THE ROTATION EFFECTS TO THE EVOLUTION OF THE B-EMISSION STARS: CASE STUDY HR 8520, HR 8402, AND HR 5941

<p align="justify">B-emission (Be) stars are B-type stars, which rotate with high velocities (100-300 km/s or more), whose spectra show, or have shown, emission lines at Hydrogen Balmer (e.g. H&#945; and H&#946;), and sometimes at neutral Helium and ionized metals. Observatio...

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Bibliographic Details
Main Author: RATNA WULANDARI - Nim: 10314014 , TRI
Format: Final Project
Language:Indonesia
Online Access:https://digilib.itb.ac.id/gdl/view/31372
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Institution: Institut Teknologi Bandung
Language: Indonesia

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https://digilib.itb.ac.id/gdl/view/31372

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