Search for variable stars in the young open cluster Stock 18

We have carried out multi-epoch deep I band photometry of the open cluster Stock 18 to search for variable stars in star forming regions. In the present study, we report identification of 28 periodic and 165 non-periodic variables stars. The periods of most of the periodic variables are in between 2...

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Main Authors: Sinha Tirthendu, Sharma Saurabh, Pandey Rakesh, Pandey A.K.
Format: Article
Language:English
Published: EDP Sciences 2017-01-01
Series:EPJ Web of Conferences
Online Access:https://doi.org/10.1051/epjconf/201715201024
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author Sinha Tirthendu
Sharma Saurabh
Pandey Rakesh
Pandey A.K.
author_facet Sinha Tirthendu
Sharma Saurabh
Pandey Rakesh
Pandey A.K.
author_sort Sinha Tirthendu
collection DOAJ
description We have carried out multi-epoch deep I band photometry of the open cluster Stock 18 to search for variable stars in star forming regions. In the present study, we report identification of 28 periodic and 165 non-periodic variables stars. The periods of most of the periodic variables are in between 2 to 20 hours and their magnitude varies between 0.05 to 0.6 mag. We have derived spectral energy distributions for 48 probable pre-main sequence variables and the average age and mass is found to be 2.7 ± 0.3 Myrs and 2.7 ± 0.2 M⊙, respectively.
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spelling doaj.art-467d21d8951347b4886f67054ca756672022-12-21T21:33:25ZengEDP SciencesEPJ Web of Conferences2100-014X2017-01-011520102410.1051/epjconf/201715201024epjconf_puls2017_01024Search for variable stars in the young open cluster Stock 18Sinha Tirthendu0Sharma Saurabh1Pandey Rakesh2Pandey A.K.3Aryabhatta Research Institute of Observational Sciences (ARIES)Aryabhatta Research Institute of Observational Sciences (ARIES)Aryabhatta Research Institute of Observational Sciences (ARIES)Aryabhatta Research Institute of Observational Sciences (ARIES)We have carried out multi-epoch deep I band photometry of the open cluster Stock 18 to search for variable stars in star forming regions. In the present study, we report identification of 28 periodic and 165 non-periodic variables stars. The periods of most of the periodic variables are in between 2 to 20 hours and their magnitude varies between 0.05 to 0.6 mag. We have derived spectral energy distributions for 48 probable pre-main sequence variables and the average age and mass is found to be 2.7 ± 0.3 Myrs and 2.7 ± 0.2 M⊙, respectively.https://doi.org/10.1051/epjconf/201715201024
spellingShingle Sinha Tirthendu
Sharma Saurabh
Pandey Rakesh
Pandey A.K.
Search for variable stars in the young open cluster Stock 18
EPJ Web of Conferences
title Search for variable stars in the young open cluster Stock 18
title_full Search for variable stars in the young open cluster Stock 18
title_fullStr Search for variable stars in the young open cluster Stock 18
title_full_unstemmed Search for variable stars in the young open cluster Stock 18
title_short Search for variable stars in the young open cluster Stock 18
title_sort search for variable stars in the young open cluster stock 18
url https://doi.org/10.1051/epjconf/201715201024
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AT sharmasaurabh searchforvariablestarsintheyoungopenclusterstock18
AT pandeyrakesh searchforvariablestarsintheyoungopenclusterstock18
AT pandeyak searchforvariablestarsintheyoungopenclusterstock18