Zobrazeno 1 - 10
of 13
pro vyhledávání: '"individual: (M 31) [Galaxies]"'
Autor:
George J. Bendo, S. Verstocken, Sébastien Viaene, Antti Tamm, S. C. Madden, P. De Vis, Matthew Smith, Maarten Baes, Médéric Boquien, Elmo Tempel, Peter Camps, Joris Blommaert, L. Spinoglio, Maud Galametz, J. A. Fernández-Ontiveros, A. Cooray, Gianfranco Gentile, Alessandro Boselli, Jacopo Fritz, I. De Looze
Publikováno v:
Viaene, S, Baes, M, Tamm, A, Tempel, E, Bendo, G, Blommaert, J A D L, Boquien, M, Boselli, A, Camps, P, Cooray, A, De Looze, I, De Vis, P, Fernández-Ontiveros, J A, Fritz, J, Galametz, M, Gentile, G, Madden, S, Smith, M W L, Spinoglio, L & Verstocken, S 2017, ' The Herschel Exploitation of Local Galaxy Andromeda (HELGA) : VII. A SKIRT radiative transfer model and insights on dust heating ', Astronomy and Astrophysics, vol. 599, A64 . https://doi.org/10.1051/0004-6361/201629251
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2017, ⟨10.1051/0004-6361/201629251⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, ⟨10.1051/0004-6361/201629251⟩
ASTRONOMY & ASTROPHYSICS
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2017, ⟨10.1051/0004-6361/201629251⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, ⟨10.1051/0004-6361/201629251⟩
ASTRONOMY & ASTROPHYSICS
The radiation of stars heats dust grains in the diffuse interstellar medium and in star-forming regions in galaxies. Modelling this interaction provides information on dust in galaxies, a vital ingredient for their evolution. It is not straightforwar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9493e49ac1722c4ae65c7257ddf2c561
https://doi.org/10.1051/0004-6361/201629251
https://doi.org/10.1051/0004-6361/201629251
Autor:
Mike Eracleous, Vallia Antoniou, Daniel Stern, Andrew Ptak, Benjamin F. Williams, William W. Craig, Finn Erland Christensen, Charles J. Hailey, Ann Hornschemeier, Steven E. Boggs, J. A. Kennea, William W. Zhang, Fiona A. Harrison, Thomas J. Maccarone, Bret D. Lehmer, M. Yukita, Andreas Zezas, K. L. Page, P. T. Boyd, Daniel R. Wik
Publikováno v:
Maccarone, T J, Yukita, M, Hornschemeier, A, Lehmer, B D, Antoniou, V, Ptak, A, Wik, D R, Zezas, A, Boyd, P, Kennea, J, Page, K L, Eracleous, M, Williams, B F, Boggs, S E, Christensen, F E, Craig, W W, Hailey, C J, Harrison, F A, Stern, D & Zhang, W W 2016, ' Demonstrating the likely neutron star nature of five M31 globular cluster sources with Swift-NuSTAR spectroscopy ', Monthly Notices of the Royal Astronomical Society, vol. 458, no. 4, pp. 3633-3643 . https://doi.org/10.1093/mnras/stw530
We present the results of a joint Swift-NuSTAR spectroscopy campaign on M31. We focus on the five brightest globular cluster X-ray sources in our fields. Two of these had previously been argued to be black hole candidates on the basis of apparent har
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f202dbdc34b65762a62d80287b478919
http://arxiv.org/abs/1603.00552
http://arxiv.org/abs/1603.00552
Autor:
Soraisam M., Gilfanov M.
Publikováno v:
SCOPUS00046361-2015-583-SID84946558869
© 2015 ESO. With the progenitors of type Ia supernovae (SNe Ia) still eluding direct detections, various types of accreting white dwarfs (WDs) have been proposed as prospective candidates. One of the possibilities are WDs undergoing unstable nuclear
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::00221be42e03dd0b8c17d0317c1f13e4
https://openrepository.ru/article?id=676555
https://openrepository.ru/article?id=676555
The objective of this work is to obtain an extinction-corrected distribution of optical surface brightness and colour indices of the large nearby galaxy M 31 using homogeneous observational data and a model for intrinsic extinction. We process the Sl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::43a56e2d6bcb70a6b9dd0c0a8546ce8b
http://arxiv.org/abs/1012.3591
http://arxiv.org/abs/1012.3591
Autor:
Henze, Martin, Pietsch, Wolfgang, Haberl, Frank, Hernanz, Margarita, Sala, Gloria, Della Valle, M., Hatzidimitriou, Despina, Rau, Arne, Hartmann, Dieter H., Greiner, Jochen, Burwitz, Vadim, Fliri, Jürgen
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
16 páginas
(Abridged) Classical novae (CNe) have recently been reported to represent the major class of supersoft X-ray sources (SSSs) in the central region of our neighbour galaxy M 31. We carried out a dedicated monitoring of the M 31 central
(Abridged) Classical novae (CNe) have recently been reported to represent the major class of supersoft X-ray sources (SSSs) in the central region of our neighbour galaxy M 31. We carried out a dedicated monitoring of the M 31 central
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::fa30e1549e822f083c7c8b6a353c73ce
http://hdl.handle.net/10261/39043
http://hdl.handle.net/10261/39043
Autor:
Dieter H. Hartmann, Michael Freyberg, Gloria Sala, Holger Stiele, Arne Rau, Margarita Hernanz, Despina Hatzidimitriou, Frank Haberl, Wolfgang Pietsch, Marina Orio, Martin Henze, Jochen Greiner
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Classical novae (CNe) have recently been reported to represent the major class of supersoft X-ray sources (SSSs) in the central area of our neighbouring galaxy M 31. This paper presents a review of results from recent X-ray observations of M 31 with
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2f2a78e750d3426b896a2c9550e26fc
http://arxiv.org/abs/0912.1247
http://arxiv.org/abs/0912.1247
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
The cosmic distance scale largely depends on distance determinations to Local Group galaxies. In this sense, the Andromeda Galaxy (M31) is a key rung to better constrain the cosmic distance ladder. A project was started in 1999 to firmly establish a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::383a851a7bd94e978bdd00d92fba9693
http://arxiv.org/abs/0911.3391
http://arxiv.org/abs/0911.3391
Autor:
M. F. Bode, Jan-Uwe Ness, Izumi Hachisu, Mariko Kato, Margarita Hernanz, Steven Williams, Gloria Sala, M. J. Darnley, Allen W. Shafter, Martin Henze
Publikováno v:
Recercat. Dipósit de la Recerca de Catalunya
instname
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
instname
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
The M 31 nova M31N 2008-12a was recently found to be a recurrent nova (RN) with a recurrence time of about 1 year. This is by far the fastest recurrence time scale of any known RNe. Our optical monitoring programme detected the predicted 2014 outburs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::216b6fc0b618ebeb1b8ddba0cce28198
https://doi.org/10.1051/0004-6361/201526028
https://doi.org/10.1051/0004-6361/201526028
Autor:
Maarten Baes, Médéric Boquien, Elmo Tempel, Laure Ciesla, O. Ł. Karczewski, Thomas Jarrett, Joris Verstappen, Walter Kieran Gear, I. De Looze, George J. Bendo, Jacopo Fritz, Matthew Smith, David A. Thilker, Sébastien Viaene, L. Spinoglio, Gianfranco Gentile, Antti Tamm, Luca Cortese, Joris Blommaert, Alessandro Boselli, T. M. Hughes
Publikováno v:
ASTRONOMY & ASTROPHYSICS
Astronomy and astrophysics, 567:A71. EDP Sciences
Astronomy and astrophysics, 567:A71. EDP Sciences
The imprints of dust-starlight interactions are visible in scaling relations between stellar characteristics, star formation parameters and dust properties. We aim to examine dust scaling relations on a sub-kpc resolution in the Andromeda galaxy (M31
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::324cf17902639fa841194711dbf6f647
https://doi.org/10.1051/0004-6361/201423534
https://doi.org/10.1051/0004-6361/201423534
Autor:
Bica, Eduardo Luiz Damiani, Jablonka, Pascale, Santos Junior, Joao Francisco Coelho dos, Alloin, Danielle Marie, Dottori, Horacio Alberto
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 star clusters G 158 and G 177, located at projected distances smaller than 1.5 kpc from the semi-stellar nucleus of M 31, show spectra extreme in absorption-line strengths, comparable to those from the nuclei of giant ellipticals or from the M 31
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3056::acef57a2483bebf55df22ce09829cfc3