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Photoelectric photometry of algol and Hamal stars / Nazirah Mohd Noris.

Photoelectric Photometry is technique of astronomy concerned with measuring flux, the most fundamental and oldest research technique and gives information about the total energy emitted by the object, its size, its temperature and other physical properties. Algol star is variable star that changes t...

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Main Author: Mohd Noris, Nazirah
Format: Student Project
Language:English
Published: 2010
Subjects:
Mathematical physics
Optics. Light
Online Access:http://ir.uitm.edu.my/id/eprint/46752/1/46752.pdf
http://ir.uitm.edu.my/id/eprint/46752/
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spelling my.uitm.ir.467522021-06-01T16:20:36Z http://ir.uitm.edu.my/id/eprint/46752/ Photoelectric photometry of algol and Hamal stars / Nazirah Mohd Noris. Mohd Noris, Nazirah Mathematical physics Optics. Light Photoelectric Photometry is technique of astronomy concerned with measuring flux, the most fundamental and oldest research technique and gives information about the total energy emitted by the object, its size, its temperature and other physical properties. Algol star is variable star that changes the brightness of the star. From the surface temperature range 10,000K until 28,000K is B spectral class, appear more bluish colour and have light curve. The comparison star is Hamal star is non- variable star that not changes brightness of the star. Hamal has the surface temperature range from 3500K to 4900K so it can classified in K spectral and the colour index (B-V) is positive value, so the star appear reddish colour. 2010 Student Project NonPeerReviewed text en http://ir.uitm.edu.my/id/eprint/46752/1/46752.pdf ID46752 Mohd Noris, Nazirah (2010) Photoelectric photometry of algol and Hamal stars / Nazirah Mohd Noris. [Student Project] (Unpublished)
institution Universiti Teknologi Mara
building Tun Abdul Razak Library
collection Institutional Repository
continent Asia
country Malaysia
content_provider Universiti Teknologi Mara
content_source UiTM Institutional Repository
url_provider http://ir.uitm.edu.my/
language English
topic Mathematical physics
Optics. Light
spellingShingle Mathematical physics
Optics. Light
Mohd Noris, Nazirah
Photoelectric photometry of algol and Hamal stars / Nazirah Mohd Noris.
description Photoelectric Photometry is technique of astronomy concerned with measuring flux, the most fundamental and oldest research technique and gives information about the total energy emitted by the object, its size, its temperature and other physical properties. Algol star is variable star that changes the brightness of the star. From the surface temperature range 10,000K until 28,000K is B spectral class, appear more bluish colour and have light curve. The comparison star is Hamal star is non- variable star that not changes brightness of the star. Hamal has the surface temperature range from 3500K to 4900K so it can classified in K spectral and the colour index (B-V) is positive value, so the star appear reddish colour.
format Student Project
author Mohd Noris, Nazirah
author_facet Mohd Noris, Nazirah
author_sort Mohd Noris, Nazirah
title Photoelectric photometry of algol and Hamal stars / Nazirah Mohd Noris.
title_short Photoelectric photometry of algol and Hamal stars / Nazirah Mohd Noris.
title_full Photoelectric photometry of algol and Hamal stars / Nazirah Mohd Noris.
title_fullStr Photoelectric photometry of algol and Hamal stars / Nazirah Mohd Noris.
title_full_unstemmed Photoelectric photometry of algol and Hamal stars / Nazirah Mohd Noris.
title_sort photoelectric photometry of algol and hamal stars / nazirah mohd noris.
publishDate 2010
url http://ir.uitm.edu.my/id/eprint/46752/1/46752.pdf
http://ir.uitm.edu.my/id/eprint/46752/
_version_ 1702172640425279488
score 13.23648

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