Mass function and dynamical study of the open clusters Berkeley 24 and Czernik 27 using ground based imaging and Gaia astrometry

D. Bisht; R. K. S. Yadav; Shashikiran Ganesh; A. K. Durgapal; G. Rangwal; J. P. U. Fynbo

doi:10.1093/mnras/sty2781

Mass function and dynamical study of the open clusters Berkeley 24 and Czernik 27 using ground based imaging and Gaia astrometry

D. Bisht, R. K. S. Yadav, Shashikiran Ganesh, A. K. Durgapal, G. Rangwal, J. P. U. Fynbo

The Cosmic Dawn Center

9 Citationer (Scopus)

Originalsprog	Engelsk
Tidsskrift	Monthly Notices of the Royal Astronomical Society
Vol/bind	482
Udgave nummer	2
Sider (fra-til)	1471-1484
ISSN	0035-8711
DOI	https://doi.org/10.1093/mnras/sty2781
Status	Udgivet - 11 jan. 2019

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10.1093/mnras/sty2781

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title = "Mass function and dynamical study of the open clusters Berkeley 24 and Czernik 27 using ground based imaging and Gaia astrometry",

keywords = "astrometry, proper motions, Hertzsprung-Russell and colour-magnitude diagrams, stars: luminosity function, mass function, open clusters and associations: individual: Berkeley 24 and Czernik 27",

author = "D. Bisht and Yadav, {R. K. S.} and Shashikiran Ganesh and Durgapal, {A. K.} and G. Rangwal and Fynbo, {J. P. U.}",

year = "2019",

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T1 - Mass function and dynamical study of the open clusters Berkeley 24 and Czernik 27 using ground based imaging and Gaia astrometry

AU - Bisht, D.

AU - Yadav, R. K. S.

AU - Ganesh, Shashikiran

AU - Durgapal, A. K.

AU - Rangwal, G.

AU - Fynbo, J. P. U.

PY - 2019/1/11

Y1 - 2019/1/11

KW - astrometry

KW - proper motions

KW - Hertzsprung-Russell and colour-magnitude diagrams

KW - stars: luminosity function, mass function

KW - open clusters and associations: individual: Berkeley 24 and Czernik 27

U2 - 10.1093/mnras/sty2781

DO - 10.1093/mnras/sty2781

M3 - Journal article

SN - 0035-8711

VL - 482

SP - 1471

EP - 1484

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 2

ER -

Mass function and dynamical study of the open clusters Berkeley 24 and Czernik 27 using ground based imaging and Gaia astrometry

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