PHOTOMETRIC AND SPECTROSCOPIC STUDIES OF AP STAR CYG V1584

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JASSUR D.

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Journal Paper

Paper Information

Journal: Iranian Journal of Physics Research Year:2001 | Volume:2 | Issue:5 Page(s): 291-299

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Information Journal Paper

Title

PHOTOMETRIC AND SPECTROSCOPIC STUDIES OF AP STAR CYG V1584

Author(s)

JASSUR D. | Issue Writer Certificate

Keywords

STARSQ3

APQ4

SILICONQ4

MAGNETIC STARSQ3

Abstract

UBV photometric observations of AP star Cyg V1584 have been presented. To find the rotational period of the star, a sinusoidal wave function has been fitted to the normal points of UBV filters. Assuming that a circular hot spot located at the magnetic pole of the star is responsible for the observed light variations, both. Physical and geometrical parameters of the spot have been determined. Finally, the angle between the magnetic and the rotational axis has been calculated from combining the spectroscopic and photometric data and the magnetic structure of the star has been discussed.

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APA: Copy

JASSUR, D.. (2001). PHOTOMETRIC AND SPECTROSCOPIC STUDIES OF AP STAR CYG V1584. IRANIAN JOURNAL OF PHYSICS RESEARCH, 2(5), 291-299. SID. https://sid.ir/paper/1796/en

Vancouver: Copy

JASSUR D.. PHOTOMETRIC AND SPECTROSCOPIC STUDIES OF AP STAR CYG V1584. IRANIAN JOURNAL OF PHYSICS RESEARCH[Internet]. 2001;2(5):291-299. Available from: https://sid.ir/paper/1796/en

IEEE: Copy

D. JASSUR, “PHOTOMETRIC AND SPECTROSCOPIC STUDIES OF AP STAR CYG V1584,” IRANIAN JOURNAL OF PHYSICS RESEARCH, vol. 2, no. 5, pp. 291–299, 2001, [Online]. Available: https://sid.ir/paper/1796/en

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