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pro vyhledávání: '"Klapkowski, Myles"'
Autor:
McQuinn, Kristen. B. W., Berg, Danielle A., Skillman, Evan D., Adams, Elizabeth, Cannon, John M., Dolphin, Andrew E., Salzer, John J., Giovanelli, Riccardo, Haynes, Martha P., Hirschauer, Alec S., Janoweicki, Steven, Klapkowski, Myles, Rhode, Katherine L.
Extremely metal-poor (XMP) galaxies are low-mass, star-forming galaxies with gas-phase oxygen abundances below 12+log(O/H) = 7.35 (~1/20 Zsun). Galaxy evolution scenarios suggest three pathways to form an XMP: (1) secular evolution at low galaxy mass
Externí odkaz:
http://arxiv.org/abs/2002.11723
Autor:
McQuinn, Kristen. B. W., Berg, Danielle A., Skillman, Evan D., Adams, Elizabeth A. K., Cannon, John M., Dolphin, Andrew E., Salzer, John J., Giovanelli, Riccardo, Haynes, Martha P., Hirschauer, Alec S., Janoweicki, Steven, Klapkowski, Myles, Rhode, Katherine L.
Publikováno v:
The Astrophysical Journal, 891(2):181. IOP PUBLISHING LTD
Extremely metal-poor (XMP) galaxies are low-mass, star-forming galaxies with gas-phase oxygen abundances below 12 + log(O/H) = 7.35 (∼ 1/20 Z⊙). Galaxy evolution scenarios suggest three pathways to form an XMP: (1) secular evolution at low galaxy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::c9e2314579998e43250c583b8e519e10
https://research.rug.nl/en/publications/c9d8ad57-d6cb-4aa2-ae2b-a4aa721cbdcb
https://research.rug.nl/en/publications/c9d8ad57-d6cb-4aa2-ae2b-a4aa721cbdcb