Virtual Journal of Nuclear Astrophysics
Edited by
Honey Arora
, Michigan State University and
Fry Fang
, University of Notre Dame
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Results 1 - 10 of 10
J1046+4047: an extremely low-metallicity dwarf star-forming galaxy with O32 = 57. (arXiv:2311.01799v1 [astro-ph.GA])
Virtual Journal - Volume 21, Issue 43 - article #18
Y. I. Izotov
(1),
T. X. Thuan
(2, 3),
N. G. Guseva
(1)
((1) Bogolyubov Institute for Theoretical Physics, National Academy of Sciences of Ukraine, Kyiv, Ukraine,
(2) Astronomy Department, University of Virginia, Charlottesville, USA,
(3) Institut d'Astrophysique de Paris, Paris, France)
http://arxiv.org/abs/2311.01799
First look with JWST spectroscopy: $z sim 8$ galaxies resemble local analogues. (arXiv:2207.10034v2 [astro-ph.GA] UPDATED)
Virtual Journal - Volume 20, Issue 29 - article #3
D. Schaerer
,
R. Marques-Chaves
,
P. Oesch
,
R. Naidu
,
L. Barrufet
,
Y. I. Izotov
,
N. G. Guseva
,
G. Brammer
http://arxiv.org/abs/2207.10034
A new determination of the primordial He abundance using the He i λ10830 Ã… emission line: cosmological implications
Virtual Journal - Volume 12, Issue 23 - article #122
Y. I. Izotov
,
T. X. Thuan
,
and
N. G. Guseva
Monthly Notices of the Royal Astronomical Society - Volume: 445, Issue: 1
Abstract
Full Text (HTML)
Full Text (PDF)
A new determination of the primordial He abundance using the HeI 10830A emission line: cosmological implications
Virtual Journal - Volume 12, Issue 22 - article #39
Y. I. Izotov
(1),
T. X. Thuan
(2),
N. G. Guseva
(1)
((1) Main Astronomical Observatory, Kyiv, Ukraine,
(2) University of Virginia, Charlottesville, USA)
arXiv.org - Astrophysics - Volume: 2014, Issue: 5 Sep
arXiv:1408.6953
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Primordial
4
He abundance: a determination based on the largest sample of H II regions with a methodology tested on model H II regions
Virtual Journal - Volume 11, Issue 45 - article #30
Y. I. Izotov
,
G. Stasińska
and
N. G. Guseva
Astronomy and Astrophysics - Volume: 558, Issue: October 2013
http://dx.doi.org/10.1051/0004-6361/201220782
Abstract
Full HTML
PDF (2.847 MB)
References
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Primordial 4He abundance: a determination based on the largest sample of HII regions with a methodology tested on model HII regions
Virtual Journal - Volume 11, Issue 32 - article #4
Y. I. Izotov
(1,2,3),
G. Stasinska
(1),
N. G. Guseva
(2 and 3)
((1) LUTH, Observatoire de Meudon, France,
(2) Main Astronomical Observatory, Kyiv, Ukraine,
(3) Max-Planck-Institut fuer Radioastronomie, Bonn, Germany)
arXiv.org - Astrophysics - Volume: 2013, Issue: 9 Aug
arXiv:1308.2100
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The chemical composition of metal-poor emission-line galaxies in the Data Release 3 of the Sloan Digital Sky Survey
Virtual Journal - Volume 3, Issue 47 - article #2
Y. I. Izotov
(1),
G. Stasinska
(2),
G. Meynet
(3),
N. G. Guseva
(1),
T. X. Thuan
(4)
((1) Main Astronomical Observatory, Kyiv, Ukraine,
(2) LUTH, Observatoire de Meudon, France,
(3) Geneva Observatory, Switzerland,
(4) University of Virginia, Charlottesville, USA)
ArXiv – Astrophysics – November 2005
astro-ph/0511644 [
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SBS 0335-052W: The Lowest-Metallicity Star-Forming Galaxy Known
Virtual Journal - Volume 3, Issue 25 - article #17
Y. I. Izotov
(1),
T. X. Thuan
(2),
N. G. Guseva
(1)
((1) Main Astronomical Observatory, Kyiv, Ukraine,
(2) Astronomy Department, University of Virginia, USA)
ArXiv - Astrophysics – June 2005
astro-ph/0506498 [
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Abundance patterns in the low-metallicity emission-line galaxies from the Early Data Release of the Sloan Digital Sky Survey
Virtual Journal - Volume 2, Issue 5 - article #31
Y. I. Izotov
,
G. Stasinska
,
N. G. Guseva
and
T. X. Thuan
Astronomy and Astrophysics - Vol. 415 No. 1
Abstract
,
Full HTML
,
PDF file (679 KB)
,
PS file (122 KB)
Abundance patterns in the low-metallicity emission-line galaxies from the Early Data Release of the Sloan Digital Sky Survey
Virtual Journal - Volume 1, Issue 20 - article #5
Y. I.
Izotov(1),
G.
Stasinska(2),
N. G.
Guseva(1),
T. X.
Thuan(3)
((1) Main Astronomical Observatory, Kyiv, Ukraine,
(2) LUTH, Observatoire de Meudon, France,
(3) University of Virginia, Charlottesville, USA)
arXiv.org - Astrophysics - Wed, 26 Nov 2003
astro-ph/0311564 [
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