Zobrazeno 1 - 10
of 162
pro vyhledávání: '"Trinh X. Thuan"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 508:2556-2574
We report the discovery of [NeV]3426 emission, in addition to HeII4686 emission, in six compact star-forming galaxies. These observations considerably increase the sample of eight such galaxies discovered earlier by our group. For four of the new gal
Autor:
Natalia G. Guseva, Daniel Schaerer, Yuri I. Izotov, Klaus J. Fricke, Anne Verhamme, Trinh X. Thuan, Gabor Worseck, John Chisholm
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 503:1734-1752
We present observations with the Cosmic Origins Spectrograph onboard the Hubble Space Telescope of nine low-mass star-forming galaxies at redshifts, z, in the range 0.3179–0.4524, with stellar masses $M_\star \, \lt $ 108 M⊙ and very high specifi
Autor:
Fabricio Ferrari, Marina Trevisan, A. Ranjan, Gary A. Mamon, Trinh X. Thuan, Leonid S. Pilyugin
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2021, 502 (4), pp.4815-4841. ⟨10.1093/mnras/staa4008⟩
Mon.Not.Roy.Astron.Soc., 2021, 502 (4), pp.4815-4841. ⟨10.1093/mnras/staa4008⟩
In the local Universe, there is a handful of dwarf compact star-forming galaxies with extremely low oxygen abundances. It has been proposed that they are young, having formed a large fraction of their stellar mass during their last few hundred Myr. H
Using the Large Binocular Telescope (LBT)/Multi-Object Dual Spectrograph (MODS), we have obtained optical spectroscopy of one of the most metal-poor dwarf star-forming galaxies (SFG) in the local Universe, J2229+2725. This galaxy with a redshift z=0.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1fda92b04c8a0636b9887b9b993d1448
http://arxiv.org/abs/2104.08035
http://arxiv.org/abs/2104.08035
Autor:
Daniel Schaerer, Klaus J. Fricke, N. G. Guseva, Christian Henkel, Yuri I. Izotov, Trinh X. Thuan
We compare the relations among various integrated characteristics of ~25,000 low-redshift (z1.5) star-forming galaxies (SFGs) with respect to oxygen abundances, stellar masses M*, far-UV absolute magnitudes M(FUV), star-formation rates SFR and specif
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::05997b270644511b1293a9a17d34428f
Publikováno v:
Mamon, G A, Trevisan, M, Thuan, T X, Gallazzi, A & Davé, R 2020, ' The frequency of very young galaxies in the local Universe-II. The view from SDSS spectra ', Monthly Notices of the Royal Astronomical Society, vol. 492, no. 2, pp. 1791-1811 . https://doi.org/10.1093/mnras/stz3556
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Only a handful of galaxies in the local Universe appear to be very young. We estimate the fraction of very young galaxies (VYGs), defined as those with more than half their stellar masses formed within the last Gyr. We fit non-parametric star formati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a31290856bcb79eadb14cb0d5dfd7499
https://www.pure.ed.ac.uk/ws/files/250789532/1912.06522v2.pdf
https://www.pure.ed.ac.uk/ws/files/250789532/1912.06522v2.pdf
Autor:
Y. I. Izotov, Ivana Orlitova, N. G. Guseva, Daniel Schaerer, Gabor Worseck, Fricke Fricke, Trinh X. Thuan, Anne Verhamme
Publikováno v:
Monthly Notices of the Royal Astronomical Society
We present observations with the Cosmic Origins Spectrograph onboard the Hubble Space Telescope of five star-forming galaxies at redshifts z in the range 0.2993-0.4317 and with high emission-line flux ratios O32=[OIII]5007/[OII]3727 ~ 8-27 aiming to
Autor:
Zhiyuan Ji, Bingjie Wang, Sophia Flury, Kirill Makan, Ricardo Amorín, Göran Östlin, Xinfeng Xu, Andrea Grazian, M. S. Oey, Trinh X. Thuan, Daniel Schaerer, Anne Jaskot, Gabor Worseck, John Chisholm, Alberto Saldana-Lopez, Mauro Giavalisco, Matthew Hayes, Henry C. Ferguson, Sanchayeeta Borthakur, Alaina Henry, Stephan R. McCandliss, Timothy M. Heckman
Publikováno v:
The Astrophysical Journal. 916:3
The relationship between galaxy characteristics and the reionization of the universe remains elusive, mainly due to the observational difficulty in accessing the Lyman continuum (LyC) at these redshifts. It is thus important to identify low-redshift
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 471:548-561
We present Large Binocular Telescope spectrophotometric observations of five low-redshift (z
16 pages, 8 figures, accepted for publication in Monthly Notices of the Royal Astronomical Society
16 pages, 8 figures, accepted for publication in Monthly Notices of the Royal Astronomical Society
Publikováno v:
Proceedings of the International Astronomical Union. 15:168-169
Interactions and mergers between dwarf galaxies are mostly gas-rich and should be marked by an intense star formation activity. But these processes, which are expected to be common at earlier times, are very difficult to observe at low redshifts. To