Zobrazeno 1 - 10
of 26
pro vyhledávání: '"Grace Telford"'
Publikováno v:
The Open Journal of Astrophysics, Vol 7 (2024)
The first few cycles of JWST have identified an overabundance of UV-bright galaxies and a general excess of UV luminosity density at $z\gtrsim10$ compared to expectations from most (pre-JWST) theoretical models. Moreover, some of the brightest high-r
Externí odkaz:
https://doaj.org/article/1248fa01c07c411e837d28ced3b8e323
Autor:
Margaret Lazzarini, Benjamin F. Williams, Meredith J. Durbin, Julianne J. Dalcanton, Adam Smercina, Eric F. Bell, Yumi Choi, Andrew Dolphin, Karoline Gilbert, Puragra Guhathakurta, Erik Rosolowsky, Evan Skillman, O. Grace Telford, Daniel Weisz
We measure the spatially resolved recent star formation history (SFH) of M33 using optical images taken with the Hubble Space Telescope as part of the Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER) survey. The area cover
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c9966c42920a8f2af7e137ac4cb3f946
http://arxiv.org/abs/2206.11393
http://arxiv.org/abs/2206.11393
Metal-poor, star-forming dwarf galaxies produce extreme nebular emission and likely played a major role in cosmic reionization. Yet, determining their contribution to the high-redshift ionizing photon budget is hampered by the lack of observations co
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5f1e33a98ba4d9cc1ef9d6ffef63d7f6
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Metal-poor massive stars dominate the light we observe from star-forming dwarf galaxies and may have produced the bulk of energetic photons that reionized the universe at high redshift. Yet, the rarity of observations of individual O stars below the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f5eac3832a1b6813c9ca340584a64adc
Autor:
M. Durbin, Benjamin F. Williams, Yumi Choi, Julianne J. Dalcanton, O. Grace Telford, Eric F. Bell, Andrew E. Dolphin
A galaxy's stellar mass-to-light ratio ($M_\star/L$) is a useful tool for converting luminosity to stellar mass ($M_\star$). However, the practical utility of $M_\star/L$ inferred from stellar population synthesis (SPS) models is limited by mismatche
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e1e3212ef609d6774b0e4adb5467aa24
http://arxiv.org/abs/2001.09157
http://arxiv.org/abs/2001.09157
Autor:
P. Kurczynski, Anna C. Wright, Grace Telford, Kartheik Iyer, Adam Broussard, Benjamin D. Johnson, Eric Gawiser, Kristen B. W. McQuinn, Charlotte Olsen
Publikováno v:
The Astrophysical Journal. 913:45
Star formation histories (SFHs) reveal physical processes that influence how galaxies form their stellar mass. We compare the SFHs of a sample of 36 nearby (D ⪅ 4 Mpc) dwarf galaxies from the ACS Nearby Galaxy Survey Treasury (ANGST), inferred from
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b37299d1781849fdf7e002bf7ee775bc
https://doi.org/10.3847/1538-4357/abf3c2
https://doi.org/10.3847/1538-4357/abf3c2
As galaxies evolve, they must enrich and exchange gas with the surrounding medium, but the timing of these processes and how much gas is involved remain poorly understood. In this work, we leverage metals as tracers of past gas flows to constrain the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8ca4bfeaacceb5c4e9b41d21d499c248
There is evidence that the well-established mass-metallicity relation in galaxies is correlated with a third parameter: star formation rate (SFR). The strength of this correlation may be used to disentangle the relative importance of different physic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::13366b81b4cf4204646b73a2d41c2ebc
Autor:
O. Grace Telford, Julianne J. Dalcanton, Benjamin F. Williams, Eric F. Bell, Andrew E. Dolphin, Meredith J. Durbin, Yumi Choi
Publikováno v:
Astrophysical Journal; 3/1/2020, Vol. 891 Issue 1, p1-1, 1p