Zobrazeno 1 - 10
of 605
pro vyhledávání: '"H I region"'
Autor:
Ridpath, Ian
Publikováno v:
A Dictionary of Astronomy, 3 ed., 2018.
Autor:
Ridpath, Ian
Publikováno v:
A Dictionary of Astronomy, 2 rev. ed., 2012.
Publikováno v:
The Astrophysical Journal. 162:L25
Hydrogen I region anomalous alpha lines recombination in Orion B spectrum, identifying carbon emitter by measured frequency separation
Autor:
Eric J. Chaisson
Publikováno v:
The Astrophysical Journal. 170:81
Autor:
Vagelpohl, Uwe
This two-volume monograph offers the first critical edition of the medieval Arabic translation of Galen's Commentary on Book 2 of the Hippocratic Epidemics produced by Hunayn ibn Ishaq (d. ca. 870). The edition is based on all extant Arabic textual w
Externí odkaz:
http://library.oapen.org/handle/20.500.12657/32359
Autor:
Vagelpohl, Uwe
This two-volume monograph offers the first critical edition of the medieval Arabic translation of Galen's Commentary on Book 2 of the Hippocratic Epidemics produced by Hunayn ibn Ishaq (d. ca. 870). The edition is based on all extant Arabic textual w
Externí odkaz:
http://library.oapen.org/handle/20.500.12657/32360
Publikováno v:
Publications of the Astronomical Society of Japan; Dec2024, Vol. 76 Issue 6, p1260-1269, 10p
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 456:4209-4218
We study the properties of HI gas in the outer regions (~2r_25) of a spiral galaxy, UGC 00439 (z = 0.01769), using HI 21-cm absorption towards different components of an extended background radio source, J0041$-$0043 (z = 1.679). The radio source exh
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 454:L51-L55
We report the detection and mapping of atomic hydrogen in HI 21cm emission from ESO 184-G82, the host galaxy of the gamma ray burst 980425. This is the first instance where HI in emission has been detected from a galaxy hosting a gamma ray burst. ESO
Autor:
Diane Cormier, D. Pequignot, Suzanne C. Madden, M.-Y. Lee, Sara R. Heap, Vianney Lebouteiller, M. W. Pakull, D. Kunth, Mélanie Chevance, F. L. Polles, Frédéric Galliano
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 602, pp.A45. ⟨10.1051/0004-6361/201629675⟩
Astron.Astrophys.
Astron.Astrophys., 2017, 602, pp.A45. ⟨10.1051/0004-6361/201629675⟩
Astron.Astrophys., 2017, 602, pp.A45. 〈10.1051/0004-6361/201629675〉
Astronomy and Astrophysics-A&A, 2017, 602, pp.A45. ⟨10.1051/0004-6361/201629675⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 602, pp.A45. ⟨10.1051/0004-6361/201629675⟩
Astron.Astrophys.
Astron.Astrophys., 2017, 602, pp.A45. ⟨10.1051/0004-6361/201629675⟩
Astron.Astrophys., 2017, 602, pp.A45. 〈10.1051/0004-6361/201629675〉
Astronomy and Astrophysics-A&A, 2017, 602, pp.A45. ⟨10.1051/0004-6361/201629675⟩
Context. The neutral interstellar medium of galaxies acts as a reservoir to fuel star formation. The dominant heating and cooling mechanisms in this phase are uncertain in extremely metal-poor star-forming galaxies. The low dust-to-gas mass ratio and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0534e0e849e49f9afa6f8ca54cf8c33e
https://hal.archives-ouvertes.fr/hal-01554830/file/aa29675-16.pdf
https://hal.archives-ouvertes.fr/hal-01554830/file/aa29675-16.pdf