Add to ORKGWe summarize the progress in identifying and observational study of extremely metal-deficient (XMD) gas-rich galaxies (BCGs, dIr and LSBDs). Due to volume limitation only the following issues are addressed: sample creation, some statistical data, Colour-Magnitude Diagrams (CMD) and ages, the case of SBS 0335-052 system, and probable evolution paths of various XMD objects
An outline is qiven of the properties of the blue compact dwarf galaxies (BCD). These properties are...
Understanding the properties of stars and gas at low metallicity is of large relevance for a variety...
Understanding the properties of stars and gas at low metallicity is of large relevance for a variety...
Extremely metal-deficient (XMD) galaxies, by definition, have oxygen abundances ≠1/10 solar, and for...
We demonstrate a successful strategy for identifying extremely metal-poor galaxies. Our preliminary ...
We present a spectroscopic study of eight extremely low-metallicity candidate emission-line galaxies...
The study of group properties of the extremely metal-deficient gas-rich local dwarfs is very promisi...
The powerful combination of MEGARA LCB mode (Integral Field Unit with 623 fibers covering a Field Of...
We report the discovery of eight new extremely metal poor galaxies [XMPGs; 12+log(O/H) lt;7.65...
Context. Extremely metal-poor (XMP) galaxies are chemically, and possibly dynamically, primordial ob...
The search for chemically unevolved galaxies remains prevalent in the nearby Universe, mostly becaus...
Extremely metal poor (XMP) galaxies are known to be very rare, despite the large numbers of low-mass...
We present the description and the first results og a new project devoted to the search for ext...
International audienceAims:The goal of this study is to measure parameters of the integrated H I emi...
We have obtained new H I observations with the 100 m Green Bank Telescope (GBT) for a sample of 29 e...
An outline is qiven of the properties of the blue compact dwarf galaxies (BCD). These properties are...
Understanding the properties of stars and gas at low metallicity is of large relevance for a variety...
Understanding the properties of stars and gas at low metallicity is of large relevance for a variety...
Extremely metal-deficient (XMD) galaxies, by definition, have oxygen abundances ≠1/10 solar, and for...
We demonstrate a successful strategy for identifying extremely metal-poor galaxies. Our preliminary ...
We present a spectroscopic study of eight extremely low-metallicity candidate emission-line galaxies...
The study of group properties of the extremely metal-deficient gas-rich local dwarfs is very promisi...
The powerful combination of MEGARA LCB mode (Integral Field Unit with 623 fibers covering a Field Of...
We report the discovery of eight new extremely metal poor galaxies [XMPGs; 12+log(O/H) lt;7.65...
Context. Extremely metal-poor (XMP) galaxies are chemically, and possibly dynamically, primordial ob...
The search for chemically unevolved galaxies remains prevalent in the nearby Universe, mostly becaus...
Extremely metal poor (XMP) galaxies are known to be very rare, despite the large numbers of low-mass...
We present the description and the first results og a new project devoted to the search for ext...
International audienceAims:The goal of this study is to measure parameters of the integrated H I emi...
We have obtained new H I observations with the 100 m Green Bank Telescope (GBT) for a sample of 29 e...
An outline is qiven of the properties of the blue compact dwarf galaxies (BCD). These properties are...
Understanding the properties of stars and gas at low metallicity is of large relevance for a variety...
Understanding the properties of stars and gas at low metallicity is of large relevance for a variety...