Zobrazeno 1 - 8
of 8
pro vyhledávání: '"F. R. N. Schneider"'
Autor:
T. Shenar, H. Sana, L. Mahy, J. Maíz Apellániz, Paul A. Crowther, M. Gromadzki, A. Herrero, N. Langer, P. Marchant, F. R. N. Schneider, K. Sen, I. Soszyński, S. Toonen
Publikováno v:
Astronomy and Astrophysics, 665:A148. EDP Sciences
We aim to hunt for massive binaries hosting a black hole companion (OB+BH) and establish the natal mass-ratio distribution of massive stars at the subsolar metallicity environment of the Large Magellanic Cloud (LMC). We use the shift-and-add grid dis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dc7d2c48523129c7cac097cdecc73c64
https://dare.uva.nl/personal/pure/en/publications/the-tarantula-massive-binary-monitoring-vi(b38eafbc-8acd-4f45-babf-91b24feec504).html
https://dare.uva.nl/personal/pure/en/publications/the-tarantula-massive-binary-monitoring-vi(b38eafbc-8acd-4f45-babf-91b24feec504).html
Autor:
H. Sana, O. H. Ramírez-Agudelo, V. Hénault-Brunet, L. Mahy, L. A. Almeida, A. de Koter, J. M. Bestenlehner, C. J. Evans, N. Langer, F. R. N. Schneider, P. A. Crowther, S. E. de Mink, A. Herrero, D. J. Lennon, M. Gieles, J. Maíz Apellániz, M. Renzo, E. Sabbi, J. Th. van Loon, J. S. Vink
Publikováno v:
Astronomy and Astrophysics, 668:L5. EDP Sciences
Two main scenarios have been proposed for origin of massive runaway stars -- dynamical ejection or release from a binary at the first core collapse -- but their relative contribution remains debated. Using two large spectroscopic campaigns towards ma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::04f3a9e0fc7a9b1b14b281e8db54923a
Publikováno v:
Astronomy & Astrophysics
Publikováno v:
Astronomy & Astrophysics
Publikováno v:
Astronomy & Astrophysics
Autor:
L. Fossati, N. Castro, M. Schöller, S. Hubrig, N. Langer, T. Morel, M. Briquet, A. Herrero, N. Przybilla, H. Sana, F. R. N. Schneider, A. de Koter, the BOB Collaboration
Publikováno v:
Astronomy & Astrophysics, 582:A45. EDP Sciences
Within the context of the collaboration "B fields in OB stars (BOB)", we used the FORS2 low-resolution spectropolarimeter to search for a magnetic field in 50 massive stars, including two reference magnetic massive stars. Because of the many controve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b64cdc438f51eee9396f1a5ee5c61417
https://dare.uva.nl/personal/pure/en/publications/b-fields-in-ob-stars-bob-lowresolution-fors2-spectropolarimetry-of-the-first-sample-of-50-massive-stars(ecaec9a9-3d72-4fd1-a7c2-2ef330f52f4c).html
https://dare.uva.nl/personal/pure/en/publications/b-fields-in-ob-stars-bob-lowresolution-fors2-spectropolarimetry-of-the-first-sample-of-50-massive-stars(ecaec9a9-3d72-4fd1-a7c2-2ef330f52f4c).html
Autor:
F. R. N. Schneider, O. H. Ramírez-Agudelo, F. Tramper, J. M. Bestenlehner, N. Castro, H. Sana, C. J. Evans, C. Sabín-Sanjulián, S. Simón-Díaz, N. Langer, L. Fossati, G. Gräfener, P. A. Crowther, S. E. de Mink, A. de Koter, M. Gieles, A. Herrero, R. G. Izzard, V. Kalari, R. S. Klessen, D. J. Lennon, L. Mahy, J. Maíz Apellániz, N. Markova, J. Th. van Loon, J. S. Vink, N. R. Walborn
Publikováno v:
Astronomy & Astrophysics
Publikováno v:
Astrophysical Journal; 5/20/2015, Vol. 805 Issue 1, p1-1, 1p