Add to ORKGTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutor: Friedrich AndersOur galaxy contains a large number of stellar open clusters still to be identified and characterized, but thanks to the new Gaia DR2 release, it is possible to identify new ones that are unknown to date and discard earlier reported clusters that turn out to be spurious. The aim of this work is to do a statistical analysis of the spatial and the age distribution as well as the completeness, using the most recent and comprehensive sample of open clusters available today from the Gaia satellite. Using these data and comparing them with old catalogues, we redetermine fundamental parameters of the cluster age function: logTbreak=8....
For over a century, open clusters have been a key tool for understanding stellar and galactic evolut...
The distribution of member stars in the surroundings of an Open Cluster (OC) can shed light on the p...
Stellar clusters are gravitationally bound groups of stars. Astronomers distinguish two types of ste...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2019, Tutor: ...
We perform a systematic reanalysis of the age distribution of Galactic open star clusters. Using a c...
[Context] The distribution of member stars in the surroundings of an open cluster (OC) can shed ligh...
The goal of my work is to address the topic of the formation and evolution of the Galactic disk thro...
In the pre-Gaia era, one of the largest collections of open clusters and their parameters was the Mi...
[Context] The improvements in the precision of the published data in Gaia EDR3 with respect to Gaia ...
Context. Data from the Gaia satellite are revolutionising our understanding of the Milky Way. With e...
Context. Determination and calibration of the ages of stars, which heavily rely on stellar evolution...
Context. The publication of the Gaia Data Release 2 (Gaia DR2) opens a new era in astronomy. It incl...
The improvements in the precision of the published data in \textit{Gaia} EDR3 with respect to \texti...
Context. Open clusters are key targets for studies of Galaxy structure and evolution, and stellar ph...
Reliable fundamental parameters of open clusters (OCs) such as distance, age, and extinction are key...
For over a century, open clusters have been a key tool for understanding stellar and galactic evolut...
The distribution of member stars in the surroundings of an Open Cluster (OC) can shed light on the p...
Stellar clusters are gravitationally bound groups of stars. Astronomers distinguish two types of ste...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2019, Tutor: ...
We perform a systematic reanalysis of the age distribution of Galactic open star clusters. Using a c...
[Context] The distribution of member stars in the surroundings of an open cluster (OC) can shed ligh...
The goal of my work is to address the topic of the formation and evolution of the Galactic disk thro...
In the pre-Gaia era, one of the largest collections of open clusters and their parameters was the Mi...
[Context] The improvements in the precision of the published data in Gaia EDR3 with respect to Gaia ...
Context. Data from the Gaia satellite are revolutionising our understanding of the Milky Way. With e...
Context. Determination and calibration of the ages of stars, which heavily rely on stellar evolution...
Context. The publication of the Gaia Data Release 2 (Gaia DR2) opens a new era in astronomy. It incl...
The improvements in the precision of the published data in \textit{Gaia} EDR3 with respect to \texti...
Context. Open clusters are key targets for studies of Galaxy structure and evolution, and stellar ph...
Reliable fundamental parameters of open clusters (OCs) such as distance, age, and extinction are key...
For over a century, open clusters have been a key tool for understanding stellar and galactic evolut...
The distribution of member stars in the surroundings of an Open Cluster (OC) can shed light on the p...
Stellar clusters are gravitationally bound groups of stars. Astronomers distinguish two types of ste...