2021
DOI: 10.3847/1538-3881/ac0138
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Abstract: We carry out a detailed photometric and kinematic study of the poorly studied sparse open clusters SAI 44 and SAI 45 using ground-based BVR c I c data supplemented by archival data from Gaia eDR3 and Pan-STARRS. The stellar memberships are determined using a statistical method based on Gaia eDR3 kinematic data, and we found 204 members in SAI 44 while only 74 members are ident… Show more

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Cited by 4 publications
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“…Several open star clusters and a few globular clusters located in our Milky-way galaxy have been observed at optical and NIR wavelengths using Devasthal observing facilities. These observations combined with GAIA kinematical and other archival data have led to the studies of star formation efficiency, age distribution, mass function and luminosity function in open star clusters (Panwar et al 2017(Panwar et al , 2022Pandey et al 2020;Maurya et al 2021;Sharma et al 2023 and references therein). Spatial structure and interstellar extinction in young open star clusters have also been studied.…”
Section: Period In Yearsmentioning
confidence: 99%
“…Several open star clusters and a few globular clusters located in our Milky-way galaxy have been observed at optical and NIR wavelengths using Devasthal observing facilities. These observations combined with GAIA kinematical and other archival data have led to the studies of star formation efficiency, age distribution, mass function and luminosity function in open star clusters (Panwar et al 2017(Panwar et al , 2022Pandey et al 2020;Maurya et al 2021;Sharma et al 2023 and references therein). Spatial structure and interstellar extinction in young open star clusters have also been studied.…”
Section: Period In Yearsmentioning
confidence: 99%