Zobrazeno 1 - 10
of 148
pro vyhledávání: '"N. P. Abel"'
Autor:
Abel, N.H., Legendre, A.M.
Publikováno v:
Journal für die reine und angewandte Mathematik; July 1830, Vol. 1830 Issue: 6 p73-80, 8p
Autor:
Poullain, N. P. Abel.
Th.--Méd.--Montpellier, 1855.
Voyez tome 1. N ° 4. Montpellier 1855.
Voyez tome 1. N ° 4. Montpellier 1855.
Externí odkaz:
http://catalogue.bnf.fr/ark:/12148/cb36922375c
We have extended the membership and determined the 3-D structure of the large (0.19 pc) HH~269 sequence of shocks in the Orion Nebula. All of the components lie along a track that is highly tilted to the plane-of-the-sky and emerge from within the Or
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0cd41d447571f24fc9ce286a904174ab
Akademický článek
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Akademický článek
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Publikováno v:
Astronomy & Astrophysics. 650:A86
Context. The Arches Cluster – Arched Filaments (AF) system is our Galaxy’s prime example of the complexity involved in the interaction between the strong radiation field of numerous OB stars and their surrounding ISM in extremely harsh environmen
Autor:
Cajori, Florian
Publikováno v:
Bulletin of the American Mathematical Society; March 1907, Vol. 13 Issue: 6 p305-306, 2p
Autor:
Diane Cormier, Sacha Hony, Remy Indebetouw, F. L. Polles, S. C. Madden, V. Lebouteiller, Min-Young Lee, Annie Hughes, J. Braine, Frédéric Galliano, Maud Galametz, M. A. Requena-Torres, Mélanie Chevance, N. P. Abel
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 632, pp.A106. ⟨10.1051/0004-6361/201936303⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 632, pp.A106. ⟨10.1051/0004-6361/201936303⟩
(abridged) The ambiguous origin of [CII] 158um in the interstellar medium complicates its use for diagnostics concerning the star-formation rate and physical conditions in photodissociation regions (PDRs). We observed the giant HII region N11 in the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::08c0840af3a0dffad0ef8025adec44f4
http://arxiv.org/abs/1911.03280
http://arxiv.org/abs/1911.03280
Autor:
F. L. Polles, I. De Looze, Diane Cormier, Sacha Hony, A. Lambert-Huyghe, N. P. Abel, Frédéric Galliano, S. C. Madden, Vianney Lebouteiller, Maud Galametz
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2019, 626, pp.A23. ⟨10.1051/0004-6361/201834457⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 626, pp.A23. ⟨10.1051/0004-6361/201834457⟩
ASTRONOMY & ASTROPHYSICS
Astronomy and Astrophysics-A&A, 2019, 626, pp.A23. ⟨10.1051/0004-6361/201834457⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 626, pp.A23. ⟨10.1051/0004-6361/201834457⟩
ASTRONOMY & ASTROPHYSICS
The sensitive infrared telescopes, Spitzer and Herschel, have been used to target low-metallicity star-forming galaxies, allowing us to investigate the properties of their interstellar medium (ISM) in unprecedented detail. Interpretation of the obser
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e14c3633eab1f548c9094f848750b9e3
https://hal.archives-ouvertes.fr/hal-02105243
https://hal.archives-ouvertes.fr/hal-02105243
We have used existing optical emission and absorption lines, [C II] emission lines, and H I absorption lines to create a new model for a Central Column of material near the Trapezium region of the Orion Nebula. This was necessary because recent high
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::80e7d54338f1f8484ef923b52b5f2194