Zobrazeno 1 - 10
of 1 067
pro vyhledávání: '"Diffuse nebulae"'
Autor:
Toalá, J. A., Arthur, S. J.
X-ray emitting diffuse nebulae around hot stars are observed to have soft-band temperatures in the narrow range [1-3]$\times10^{6}$ K, independent of the stellar wind parameters and the evolutionary stage of the central star. We discuss the origin of
Externí odkaz:
http://arxiv.org/abs/1804.10244
Publikováno v:
Publications of the Astronomical Society of the Pacific, 1982 Jun 01. 94(559), 444-452.
Externí odkaz:
https://www.jstor.org/stable/40677977
Autor:
Osterbrock, Donald E.
Publikováno v:
Publications of the Astronomical Society of the Pacific, 1967 Dec 01. 79(471), 523-545.
Externí odkaz:
https://www.jstor.org/stable/40674526
Autor:
Osterbrock, Donald E.
Publikováno v:
Publications of the Astronomical Society of the Pacific, 1959 Feb 01. 71(418), 23-27.
Externí odkaz:
https://www.jstor.org/stable/40673431
Publikováno v:
Publications of the Astronomical Society of the Pacific, 1947 Jun 01. 59(348), 139-142.
Externí odkaz:
https://www.jstor.org/stable/40671798
Autor:
Lundmark, Knut
Publikováno v:
Publications of the Astronomical Society of the Pacific, 1922 Feb 01. 34(197), 40-49.
Externí odkaz:
https://www.jstor.org/stable/40668552
Autor:
RUSSELL, HENRY NORRIS
Publikováno v:
Scientific American, 1938 Aug 01. 159(2), 74-75.
Externí odkaz:
https://www.jstor.org/stable/24955407
Autor:
Kurchakov, A.V.
Publikováno v:
Astronomical & Astrophysical Transactions. 2003, Vol. 22 Issue 2, p117. 7p.
Autor:
Jesús A. Toalá, Sarah Jane Arthur
X-ray emitting diffuse nebulae around hot stars are observed to have soft-band temperatures in the narrow range [1-3]$\times10^{6}$ K, independent of the stellar wind parameters and the evolutionary stage of the central star. We discuss the origin of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0c8a09c67dc32eb0a60756de8d2bf44a
http://arxiv.org/abs/1804.10244
http://arxiv.org/abs/1804.10244
Applying the Velocity Gradient Technique in NGC 1333: Comparison with Dust Polarization Observations
Publikováno v:
The Astrophysical Journal, Vol 976, Iss 2, p 254 (2024)
Magnetic fields ( B -fields) are ubiquitous in the interstellar medium (ISM), and they play an essential role in the formation of molecular clouds and subsequent star formation. However, B -fields in interstellar environments remain challenging to me
Externí odkaz:
https://doaj.org/article/90391a4b032c433a8064734498b50b5b