Carbon monoxide in an extremely metal-poor galaxy
Extremely metal-poor galaxies in the local universe are the best analogues to investigating the interstellar medium at a quasi-primitive environment in the early universe. Here, the authors detect CO emission in a galaxy at 7% solar metallicity, offering direct evidence for the presence of molecular...
Main Authors: | Yong Shi, Junzhi Wang, Zhi-Yu Zhang, Yu Gao, Cai-Na Hao, Xiao-Yang Xia, Qiusheng Gu |
---|---|
Format: | Article |
Language: | English |
Published: |
Nature Publishing Group
2016-12-01
|
Series: | Nature Communications |
Online Access: | https://doi.org/10.1038/ncomms13789 |
Similar Items
-
HIGH-RESOLUTION SPECTROSCOPY OF EXTREMELY METAL-POOR STARS IN THE LEAST EVOLVED GALAXIES: BOOTES II
by: Simon, Joshua D., et al.
Published: (2016) -
CARBON-ENHANCED METAL-POOR STAR FREQUENCIES IN THE GALAXY: CORRECTIONS FOR THE EFFECT OF EVOLUTIONARY STATUS ON CARBON ABUNDANCES
by: Placco, Vinicius M., et al.
Published: (2015) -
On the Abundances of Li, Be and O in Metal-Poor Stars in the Galaxy
by: García Pérez, Ana Elia
Published: (2005) -
Detection of a Population of Carbon-enhanced Metal-poor Stars in the Sculptor Dwarf Spheroidal Galaxy*
by: Simon, Joshua D., et al.
Published: (2018) -
Features of Carbon Monoxide Poisoning in China.
by: Juan Xue, et al.
Published: (2013-10-01)