A Young Star Cluster in the Leo a Galaxy

We report a serendipitous discovery of a star cluster in the dwarf irregular galaxy Leo A. Young age (~28 Myr) and low mass (~510 M⊙) estimates are based on the isochrone fit assuming a metallicity derived for HII regions (Z = 0.0007). The color-magnitude diagrams of the stars, located in and around...

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Main Authors: Stonkutė R., Narbutis D., Bridžius A., Leščinskaitė A., Vansevičius V.
Format: Article
Language:English
Published: De Gruyter 2015-09-01
Series:Open Astronomy
Subjects:
Online Access:https://doi.org/10.1515/astro-2017-0229
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author Stonkutė R.
Narbutis D.
Bridžius A.
Leščinskaitė A.
Vansevičius V.
author_facet Stonkutė R.
Narbutis D.
Bridžius A.
Leščinskaitė A.
Vansevičius V.
author_sort Stonkutė R.
collection DOAJ
description We report a serendipitous discovery of a star cluster in the dwarf irregular galaxy Leo A. Young age (~28 Myr) and low mass (~510 M⊙) estimates are based on the isochrone fit assuming a metallicity derived for HII regions (Z = 0.0007). The color-magnitude diagrams of the stars, located in and around the cluster area, and the results of aperture photometry of the cluster itself are presented.
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spelling doaj.art-709dda6307104d399a752994fa00755a2022-12-21T18:31:06ZengDe GruyterOpen Astronomy2543-63762015-09-0124329329710.1515/astro-2017-0229astro-2017-0229A Young Star Cluster in the Leo a GalaxyStonkutė R.0Narbutis D.1Bridžius A.2Leščinskaitė A.3Vansevičius V.4 Center for Physical Sciences and Technology, Savanorių 231, Vilnius LT-02300, Lithuania Center for Physical Sciences and Technology, Savanorių 231, Vilnius LT-02300, Lithuania Center for Physical Sciences and Technology, Savanorių 231, Vilnius LT-02300, Lithuania Center for Physical Sciences and Technology, Savanorių 231, Vilnius LT-02300, Lithuania Center for Physical Sciences and Technology, Savanorių 231, Vilnius LT-02300, LithuaniaWe report a serendipitous discovery of a star cluster in the dwarf irregular galaxy Leo A. Young age (~28 Myr) and low mass (~510 M⊙) estimates are based on the isochrone fit assuming a metallicity derived for HII regions (Z = 0.0007). The color-magnitude diagrams of the stars, located in and around the cluster area, and the results of aperture photometry of the cluster itself are presented.https://doi.org/10.1515/astro-2017-0229galaxies: dwarf, irregulargalaxies: individual (leo a)galaxies: star clusters
spellingShingle Stonkutė R.
Narbutis D.
Bridžius A.
Leščinskaitė A.
Vansevičius V.
A Young Star Cluster in the Leo a Galaxy
Open Astronomy
galaxies: dwarf, irregular
galaxies: individual (leo a)
galaxies: star clusters
title A Young Star Cluster in the Leo a Galaxy
title_full A Young Star Cluster in the Leo a Galaxy
title_fullStr A Young Star Cluster in the Leo a Galaxy
title_full_unstemmed A Young Star Cluster in the Leo a Galaxy
title_short A Young Star Cluster in the Leo a Galaxy
title_sort young star cluster in the leo a galaxy
topic galaxies: dwarf, irregular
galaxies: individual (leo a)
galaxies: star clusters
url https://doi.org/10.1515/astro-2017-0229
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AT narbutisd ayoungstarclusterintheleoagalaxy
AT bridziusa ayoungstarclusterintheleoagalaxy
AT lescinskaitea ayoungstarclusterintheleoagalaxy
AT vanseviciusv ayoungstarclusterintheleoagalaxy
AT stonkuter youngstarclusterintheleoagalaxy
AT narbutisd youngstarclusterintheleoagalaxy
AT bridziusa youngstarclusterintheleoagalaxy
AT lescinskaitea youngstarclusterintheleoagalaxy
AT vanseviciusv youngstarclusterintheleoagalaxy