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2016 | 42 | 132-142
Article title

How to Plot the H-R Diagram and Use its Applications

Content
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Languages of publication
EN
Abstracts
EN
In this study, we sought to explain how the stars who due to their physical features classified. In following, we explain more of what outcomes can be extracted category. However, we must consider that the physical characteristics of stars, clusters of stars in the universe will have an important role in finding distribution patternof stars
Year
Volume
42
Pages
132-142
Physical description
Contributors
  • Department of Physics, Faculty of Basic Sciences, University of Neyshabur, P. O. Box 9318713331, Neyshabur, Iran, sd-sadatian@um.ac.ir
References
  • [1] Porter, Roy (2003). The Cambridge History of Science. Cambridge, UK: Cambridge University Press. p. 518. ISBN 978-0-521-57243-9.
  • [2] S.D. Sadatian, Is Time Inhomogeneous?, International Letters of Chemistry, Physics and Astronomy 13(2) (2014) 155-159.
  • [3] S.D. Sadatian, A Anvari, F(T) Dark Energy Model and SNe Data, World Scientific News 12 (2015) 12-26.
  • [4] S.D. Sadatian, Orderly Disorder in modern Physics, International Letters of Chemistry, Physics and Astronomy 9(2) (2015) 163-172.
  • [5] S.D. Sadatian, Possibility of Stars Energy Mechanism on the Earth, International Letters of Chemistry, Physics and Astronomy 6 (2015) 42-49.
  • [6] S.D. Sadatian, Introduce of Generalized Uncertainty Principle; International Letters of Chemistry, Physics and Astronomy 20(1) (2014) 10-20 (2014).
Document Type
article
Publication order reference
Identifiers
YADDA identifier
bwmeta1.element.psjd-721aa0f2-a59b-410b-bfe6-ae4aba3df3c7
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