The Gaia hybrid catalog: a leverage to find Galactic structures

2014 ◽  
Vol 67-68 ◽  
pp. 371-372
Author(s):  
M. Fouesneau ◽  
C.A.L. Bailer-Jones
Keyword(s):  
2012 ◽  
Vol 8 (S295) ◽  
pp. 323-323
Author(s):  
Zhi-Min Zhou ◽  
Chen Cao ◽  
Hong Wu

AbstractStellar bars are important internal drivers of the secular evolution of disk galaxies. Using a sample of nearby barred galaxies with weak and strong bars, we evaluate the correlations between star formation properties in different galactic structures and their associated bars, and try to interpret the complex process of bar-driven secular evolution. We find that weaker bars tend to associate with lower concentrical star formation activities, while stronger bars appear to have large scatter in the distribution of the global star formation activities. In general, the star formation activities in early- and late-type galaxies have different behavior, with similar star formation rate density distributions. In addition, there are only weak trends toward increased star formation activities in bulges and galaxies with stronger bars, which is consistent with previous works. Our results suggest that the different stages of the evolutionary sequence and many factors besides bars may contribute to the complexity of this process. Furthermore, significant correlations are found between the star formation activities in different galactic structures, in which barred galaxies with intense star formation in bulges tend to also have active star formation in their bars and disks. Most bulges have higher star formation densities than their associated bars and disks, indicating the presence of bar-driven evolution. Therefore, we derived a possible criterion (Figure 1) to quantify the different stages of a bar-driven evolutionary sequence. Future work is needed to improve on the uncertainties of this study.


2015 ◽  
Vol 11 (S317) ◽  
pp. 284-285
Author(s):  
Kyungwon Chun ◽  
Jihye Shin ◽  
Sungsoo S. Kim

AbstractIn this study, we aim to trace formation of the primordial globular cluster, ultra faint dwarf galaxy, and ultra compact dwarf in a cosmological context of a high-resolution hydrodynamic zoom-in simulation. We show that the baryon-dominated systems have experienced more interactions with the mini halos before infalling to the main halo.


2013 ◽  
Vol 9 (S298) ◽  
pp. 417-417
Author(s):  
L. Leedjärv

AbstractThe Gaia mission is expected to provide a total number of symbiotic stars in the Galaxy and their membership in stellar populations. Symbiotic stars with distinct emission lines in their spectra can be used as test objects in the analysis of Gaia data on peculiar stars.


2004 ◽  
Vol 48 (11) ◽  
pp. 877-899 ◽  
Author(s):  
V. L. Polyachenko ◽  
E. V. Polyachenko

Galaxies ◽  
2018 ◽  
Vol 6 (1) ◽  
pp. 22 ◽  
Author(s):  
Salvatore Capozziello ◽  
Duško Borka ◽  
Vesna Borka Jovanović ◽  
Predrag Jovanović
Keyword(s):  

1980 ◽  
Vol 85 ◽  
pp. 369-383 ◽  
Author(s):  
René Racine

The study of globular cluster systems is very important. Because these systems are so old, their investigation is a form of archeo-astronomy whereby a slow and, at times, tedious gathering of fragmentary data laboriously uncovers the skeleton of early galactic structures. Our theories and our imagination can then try to put some flesh on these bones in attempts to visualize what these early inhabitants of the Universe might have looked like.


1981 ◽  
Vol 32 (15) ◽  
pp. 411-414 ◽  
Author(s):  
A. Crollalanza ◽  
Gao Jian Gong ◽  
E. Euffini

2020 ◽  
Vol 2020 (10) ◽  
pp. 031-031 ◽  
Author(s):  
Thomas Lacroix ◽  
Arturo Núñez-Castiñeyra ◽  
Martin Stref ◽  
Julien Lavalle ◽  
Emmanuel Nezri

2017 ◽  
Author(s):  
Henrike Fleischhack ◽  
Hugo Ayala Solares ◽  
Petra Huentemeyer ◽  
Matthew Coel ◽  

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