Zobrazeno 1 - 5
of 5
pro vyhledávání: '"individual (M 83) [Galaxies]"'
Reconnection heating has been considered as a potential source of the heating of the interstellar medium. In some galaxies, significant polarised radio emission has been found between the spiral arms. This emission has a form of `magnetic arms' that
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb9ed844420c468e30c850700d0242bd
Autor:
Julia Kamenetzky, Ronin Wu, Frederic Bournaud, Christine D. Wilson, Aurélie Rémy-Ruyer, M.-Y. Lee, Maximilien R. P. Schirm, S. Hony, Miguel Pereira-Santaella, Naseem Rangwala, I. De Looze, Maarten Baes, Diane Cormier, A. Boselli, P. Panuzzo, Jason Glenn, Thomas M. Hughes, Vianney Lebouteiller, S. C. Madden, P. R. Maloney, Luigi Spinoglio, Frédéric Galliano
Publikováno v:
ASTRONOMY & ASTROPHYSICS
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 575, pp.A88. ⟨10.1051/0004-6361/201423847⟩
Astronomy and Astrophysics-A&A, 2015, 575, pp.A88. ⟨10.1051/0004-6361/201423847⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 575, pp.A88. ⟨10.1051/0004-6361/201423847⟩
Astronomy and Astrophysics-A&A, 2015, 575, pp.A88. ⟨10.1051/0004-6361/201423847⟩
Since the launch of the Herschel Space Observatory, our understanding about the photo-dissociation regions (PDR) has taken a step forward. In the bandwidth of the Fourier Transform Spectrometer (FTS) of the Spectral and Photometric Imaging REceiver (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9af4125a57733ffdc93569d1b356dace
http://arxiv.org/abs/1412.1880
http://arxiv.org/abs/1412.1880
Publikováno v:
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
The Fanaroff-Riley II radio source J133658.3-295105, which is also an X-ray source, appears to be projected onto the disk of the barred-spiral galaxy M83 at about 60´´ from the galaxy´s optical nucleus. J133658.3-295105 and its radio lobes are ali
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d9820c3d05d87a69f6c0212acf2fe7c
Publikováno v:
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
We present Gemini optical imaging and spectroscopy of the radio source J 133658.3–295105. This source has been suggested to be the core of an FR II radio source with two detected lobes. J 133658.3–295105 and its lobes are aligned with the optical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3056::92a888cd334b13f05caf0fbf9c31f009
Autor:
Monica Tosi, Angeles I. Díaz
Publikováno v:
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
instname
One of the possible applications of stellar nucleosynthesis models is the study of the behaviour of chemical elements during the evolution of galaxies. The combination of correct models of stellar nucleosynthesis and of galactic evolution should allo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::92eea6565f119e8d45de2b9aef310c27
https://doi.org/10.1093/mnras/208.2.365
https://doi.org/10.1093/mnras/208.2.365
