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@article{1778457,
author = {Dias, W. S. and Monteiro, H. and Moitinho, A. and Lepine, J. R. D. and Carraro, G. and Paunzen, Ernst and Alessi, B. and Villela, L.},
article_number = {1},
doi = {http://dx.doi.org/10.1093/mnras/stab770},
keywords = {Galaxy: open clusters and associations: general},
language = {eng},
issn = {0035-8711},
journal = {Monthly Notices of the Royal Astronomical Society},
title = {Updated parameters of 1743 open clusters based on Gaia DR2},
url = {https://doi.org/10.1093/mnras/stab770},
volume = {504},
year = {2021}
}
TY - JOUR
ID - 1778457
AU - Dias, W. S. - Monteiro, H. - Moitinho, A. - Lepine, J. R. D. - Carraro, G. - Paunzen, Ernst - Alessi, B. - Villela, L.
PY - 2021
TI - Updated parameters of 1743 open clusters based on Gaia DR2
JF - Monthly Notices of the Royal Astronomical Society
VL - 504
IS - 1
SP - 356-371
EP - 356-371
PB - Oxford University Press
SN - 00358711
KW - Galaxy: open clusters and associations: general
UR - https://doi.org/10.1093/mnras/stab770
N2 - In this study, we follow up our recent paper (Monteiro et al. 2020) and present a homogeneous sample of fundamental parameters of open clusters in our Galaxy, entirely based on Gaia DR2 data. We used published membership probability of the stars derived from Gaia DR2 data and applied our isochrone fitting code, updated as in Monteiro et al. (2020), to GBP and GRPGaia DR2 data for member stars. In doing this, we take into account the nominal errors in the data and derive distance, age, and extinction of each cluster. This work therefore provides parameters for 1743 open clusters and, as a by-product, a list of likely not physical or dubious open clusters is provided as well for future investigations. Furthermore, it was possible to estimate the mean radial velocity of 831 clusters (198 of which are new and unpublished so far), using stellar radial velocities from Gaia DR2 catalogue. By comparing the open cluster distances obtained from isochrone fitting with those obtained from a maximum likelihood estimate of individual member parallaxes, we found a systematic offset of (−0.05 ± 0.04) mas.
ER -
DIAS, W. S., H. MONTEIRO, A. MOITINHO, J. R. D. LEPINE, G. CARRARO, Ernst PAUNZEN, B. ALESSI a L. VILLELA. Updated parameters of 1743 open clusters based on Gaia DR2. \textit{Monthly Notices of the Royal Astronomical Society}. Oxford University Press, 2021, roč.~504, č.~1, s.~356-371. ISSN~0035-8711. Dostupné z: https://dx.doi.org/10.1093/mnras/stab770.
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