Differential Time-Series CCD Photometry of BL Camelopardalis

Differential time-series observations of BL Camelopardalis classified as a double mode SX Phoenicis type variable were secured with a charge coupled device. The observed photometric data was reduced using the IRAF Package and the differential magnitudes were obtained through aperture photometry. The...

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Main Authors: Chulhee Kim, Eun-Jeung Sim
Format: Article
Language:English
Published: The Korean Space Science Society 1999-12-01
Series:Journal of Astronomy and Space Sciences
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1999/v16n2/OJOOBS_1999_v16n2_241.pdf
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author Chulhee Kim
Eun-Jeung Sim
author_facet Chulhee Kim
Eun-Jeung Sim
author_sort Chulhee Kim
collection DOAJ
description Differential time-series observations of BL Camelopardalis classified as a double mode SX Phoenicis type variable were secured with a charge coupled device. The observed photometric data was reduced using the IRAF Package and the differential magnitudes were obtained through aperture photometry. The periods of BL Cam were analyzed with the Generalized Least-Square Method by Vanicek (1971) and the Fourier Decomposition Method. It was found that the first and second period of BL Cam were 0.0391 day and 0.0317 day respectively which lead the period ratio of P1/P0 = 0.81. This period ratio is much different from 0.78 determined by other investigators and also much more larger than that of other double-mode SX Phe type variables. In addition, this period ratio is much different from the value expected from the relation between the metallicity and period ratio. From these results, it can be confirmed that BL Cam is the most extreme case among all double-mode SX Phe type variables.
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spelling doaj.art-c4ad39bd04714d1eb4d6dee48fbc3c7b2024-01-02T17:39:57ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14091999-12-01162241254Differential Time-Series CCD Photometry of BL CamelopardalisChulhee Kim0Eun-Jeung Sim1Department of Earth Science Education, Chonbuk National UniversityDepartment of Earth Science Education, Chonbuk National UniversityDifferential time-series observations of BL Camelopardalis classified as a double mode SX Phoenicis type variable were secured with a charge coupled device. The observed photometric data was reduced using the IRAF Package and the differential magnitudes were obtained through aperture photometry. The periods of BL Cam were analyzed with the Generalized Least-Square Method by Vanicek (1971) and the Fourier Decomposition Method. It was found that the first and second period of BL Cam were 0.0391 day and 0.0317 day respectively which lead the period ratio of P1/P0 = 0.81. This period ratio is much different from 0.78 determined by other investigators and also much more larger than that of other double-mode SX Phe type variables. In addition, this period ratio is much different from the value expected from the relation between the metallicity and period ratio. From these results, it can be confirmed that BL Cam is the most extreme case among all double-mode SX Phe type variables.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1999/v16n2/OJOOBS_1999_v16n2_241.pdf
spellingShingle Chulhee Kim
Eun-Jeung Sim
Differential Time-Series CCD Photometry of BL Camelopardalis
Journal of Astronomy and Space Sciences
title Differential Time-Series CCD Photometry of BL Camelopardalis
title_full Differential Time-Series CCD Photometry of BL Camelopardalis
title_fullStr Differential Time-Series CCD Photometry of BL Camelopardalis
title_full_unstemmed Differential Time-Series CCD Photometry of BL Camelopardalis
title_short Differential Time-Series CCD Photometry of BL Camelopardalis
title_sort differential time series ccd photometry of bl camelopardalis
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1999/v16n2/OJOOBS_1999_v16n2_241.pdf
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