A new spectroscopic binary BD +<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si37.gif" overflow="scroll"><mml:mrow><mml:mn>38</mml:mn><mml:mi>°</mml:mi><mml:mn>2777</mml:mn></mml:mrow></mml:math> in the field of doubtful open cluster DOL–DZIM 5

Kazlauskas, A.; Sperauskas, J.; Boyle, Richard P.

doi:10.1016/j.newast.2012.07.003

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2018

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“…1. Kazlauskas et al 2013 andDias et al 2014 mentioned some few astrometric information about the cluster. No real photometric data has been published for Dolidze 41 to date except the study of Tadross & Nasser 2010, hereafter TN (2010.…”

Section: Introductionmentioning

confidence: 99%

The simplest way to get a cluster’s parameters in the Gaia era (Dolidze 41)

Tadross

2018

Res. Astron. Astrophys.

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The astro-photometric parameters of the open star cluster Dolidze 41, which located in the constellation of Cygnus, have been investigated using the Gaia-ESO DR2 large Survey merging with the near Infrared Two Micron All Sky Survey 2MASS database. The radial density distribution (limited, core and tidal radii), color-magnitude diagrams, the galactocentric coordinates, distances, color excess, and age of Dolidze 41 are presented. Thanks to Gaia DR2 astrometry, which help us to define the membership of the cluster stars easily. The luminosity & mass functions, the entire luminosity & mass, and the repose time of the cluster have been estimated as well.

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Section: Introductionmentioning

confidence: 99%

The simplest way to get a cluster’s parameters in the Gaia era (Dolidze 41)

Tadross

2018

Res. Astron. Astrophys.

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A new spectroscopic binary BD +38°2777 in the field of doubtful open cluster DOL–DZIM 5

Cited by 1 publication

References 19 publications

The simplest way to get a cluster’s parameters in the Gaia era (Dolidze 41)

The simplest way to get a cluster’s parameters in the Gaia era (Dolidze 41)

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