scholarly journals Dust-to-gas ratio and star formation history of blue compact dwarf galaxies

2002 ◽  
Vol 388 (2) ◽  
pp. 439-445 ◽  
Author(s):  
H. Hirashita ◽  
Y. Y. Tajiri ◽  
H. Kamaya
1983 ◽  
Vol 6 ◽  
pp. 179-186
Author(s):  
J. R. Mould

This review will take the linear view of the history of stellar systems. Thus the last billion years of a dwarf galaxy’s development receives no special attention. A considerable amount of information has recently come to light on the intermediate age populations of dwarf galaxies.


2014 ◽  
Vol 789 (2) ◽  
pp. 96 ◽  
Author(s):  
Hakim Atek ◽  
Jean-Paul Kneib ◽  
Camilla Pacifici ◽  
Matthew Malkan ◽  
Stephane Charlot ◽  
...  

2018 ◽  
Vol 14 (S344) ◽  
pp. 429-436
Author(s):  
Hakim Atek

AbstractDwarf galaxies represent the dominant population at high redshift and they most likely contributed in great part to star formation history of the Universe and cosmic reionization. The importance of dwarf galaxies at high redshift has been mostly recognized in the last decade due to large progress in observing facilities allowing deep galaxy surveys to identify low-mass galaxies. This population appear to have extreme emission lines and ionizing properties that challenge stellar population models. Star formation follows a stochastic process in these galaxies, which has important implication on the ionizing photon production and its escape fraction whose measurements are challenging for both simulations and observations. Outstanding questions include: what are the physical properties at the origin of such extreme properties? What are the smallest dark matter halos that host star formation? Are dwarf galaxies responsible for cosmic reionization?


2013 ◽  
Vol 778 (2) ◽  
pp. 103 ◽  
Author(s):  
Sebastian L. Hidalgo ◽  
Matteo Monelli ◽  
Antonio Aparicio ◽  
Carme Gallart ◽  
Evan D. Skillman ◽  
...  

2021 ◽  
Vol 909 (2) ◽  
pp. 192 ◽  
Author(s):  
C. Gallart ◽  
M. Monelli ◽  
T. Ruiz-Lara ◽  
A. Calamida ◽  
S. Cassisi ◽  
...  

2016 ◽  
Vol 11 (S321) ◽  
pp. 132-132
Author(s):  
Sylvain Fouquet ◽  
Ewa L. Łokas ◽  
Andrés del Pino

AbstractWe present an evolutionary model for the origin of Andromeda II, a dwarf spheroidal satellite of M31. The model is an extension of the scenario proposed by Łokas et al. (2014) involving a major merger between two gas-rich disky dwarf galaxies.


2010 ◽  
Vol 2010 ◽  
pp. 1-5 ◽  
Author(s):  
Kentaro Nagamine

We examine the past and current work on the star formation (SF) histories of dwarf galaxies in cosmological hydrodynamic simulations. The results obtained from different numerical methods are still somewhat mixed, but the differences are understandable if we consider the numerical and resolution effects. It remains a challenge to simulate the episodic nature of SF history in dwarf galaxies at late times within the cosmological context of a cold dark matter model. More work is needed to solve the mysteries of SF history of dwarf galaxies employing large-scale hydrodynamic simulations on the next generation of supercomputers.


2017 ◽  
Vol 605 ◽  
pp. A54 ◽  
Author(s):  
Jinhyub Kim ◽  
Aeree Chung ◽  
O. Ivy Wong ◽  
Bumhyun Lee ◽  
Eon-Chang Sung ◽  
...  

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