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of 121
pro vyhledávání: '"W.-J. de Wit"'
Autor:
Evgenia Koumpia, M Koutoulaki, W-J de Wit, R D Oudmaijer, A J Frost, S L Lumsden, J M Pittard
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 519:L51-L56
With steady observational advances, the formation of massive stars is being understood in more detail. Numerical models are converging on a scenario where accretion discs play a key role. Direct observational evidence of such discs at a few au scales
Akademický článek
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Autor:
E. Bordier, A. J. Frost, H. Sana, M. Reggiani, A. Mérand, A. Rainot, M. C. Ramírez-Tannus, W. J. de Wit
Spectroscopic multiplicity surveys of O stars in young clusters and OB associations have revealed that a large portion ($\sim$ 70%) of these massive stars (M$_{i}$ $\gt$ 15 $M_{\odot}$) belong to close and short-period binaries (physical separation d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::39cc159790aaf74882d111d7417d767d
https://lirias.kuleuven.be/handle/20.500.12942/700304
https://lirias.kuleuven.be/handle/20.500.12942/700304
Autor:
V. Graham, N. L. J. Cox, Eric Lagadec, C. Wichittanakom, R. D. Oudmaijer, F. Millour, G. Banyard, S. H. J. Wallstrom, John H. Black, Albert A. Zijlstra, E. Koumpia, Ryszard Szczerba, Sebastien Muller, K. M. Ababakr, H. Van Winckel, W. J. de Wit, Michel Hillen, Jacco Vink
Context. The fate of a massive star during the latest stages of its evolution is highly dependent on its mass-loss rate/geometry and therefore knowing the geometry of the circumstellar material close to the star and its surroundings is crucial. Aims.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bf4534a3f31ec47164176c78ea74f4bf
Massive stars (M>8Mdot) hold huge influence in the cosmos, affecting scales from their own stellar environment and to whole galaxies. Despite their importance, the formation of massive stars is poorly understood as they are deeply embedded, distant a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4c852eb1d4572db21a49a865737fb6ff
Autor:
Giuliano Pignata, Peter Scicluna, Neil M. Phillips, Andrea Mehner, W. J. de Wit, Dietrich Baade, C. Agliozzo, Daniel Asmus, Francisca Kemper
(Shortened) Luminous blue variable stars (LBVs) form dust as a result of episodic, violent mass loss. To investigate their contribution as dust producers in the Magellanic Clouds, we analyse 31 LBVs from a recent census. We built a maximally complete
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::94c754302a92e23d213e0bce929df8cf
https://eprints.soton.ac.uk/453215/
https://eprints.soton.ac.uk/453215/
Autor:
John D. Ilee, M. Vioque, W. J. de Wit, Rene D. Oudmaijer, I. Mendigutía, P. Marcos-Arenal, Benjamin Montesinos, J. Guzmán-Díaz, C. Wichittanakom, E. Koumpia
Publikováno v:
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname
instname
(Abridged:) It has been hypothesized that the location of Herbig Ae/Be stars (HAeBes) within the empirical relation between the inner disk radius (r$_{in}$), inferred from K-band interferometry, and the stellar luminosity (L$_*$), is related to the p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::908fad95adfbf058024bc32d978e3943
https://www.aanda.org/articles/aa/full_html/2021/08/aa40724-21/aa40724-21.html
https://www.aanda.org/articles/aa/full_html/2021/08/aa40724-21/aa40724-21.html
Autor:
Th. Rivinius, C. M. P. Russell, A. Domiciano de Souza, Uwe Beckmann, Lucas Labadie, F. Allouche, P. Cruzalèbes, Sylvie Robbe-Dubois, Antoine Mérand, William C. Danchi, A. F. J. Moffat, Kenji Hamaguchi, Michael F. Corcoran, József Varga, Alexis Matter, Thomas I. Madura, Stephane Lagarde, Sebastian Wolf, Anthony Meilland, Walter Jaffe, Paul Bristow, T. R. Gull, Felix Bettonvil, D. A. Espinoza-Galeas, Jose H. Groh, J. C. Augereau, Carsten Dominik, W. J. de Wit, Markus Schöller, J. Leftley, V. Hocdé, Uwe Graser, R. van Boekel, F. Navarete, L. Klarmann, K. Ohnaka, Leonard Burtscher, Th. Henning, Karl-Heinz Hofmann, Augusto Damineli, Ian R. Stevens, C. Connot, Klaus Meisenheimer, Stefan Kraus, Patrick W. Morris, G. Yoffe, Michiel R. Hogerheijde, Romain Petrov, Ph. Berio, M. Heininger, Henrik Hartman, J. W. Isbell, Markus Wittkowski, Eric Pantin, E. Kokoulina, J. Drevon, Julien Woillez, L. B. F. M. Waters, E. Nußbaum, Dieter Schertl, Bruno Lopez, Alexander Kreplin, Gerd Weigelt, Florentin Millour, D. J. Hillier, J. Hron, M. Lehmitz, V. Gámez Rosas, J. Sanchez-Bermudez, Noel D. Richardson, C. A. Hummel, Claudia Paladini, Andrea Mehner, Farrokh Vakili, Andreas Glindemann, P. Antonelli, C. Leinert, Gérard Zins, Philippe Stee
Publikováno v:
Astronomy & Astrophysics, 652:A140. EDP Sciences
Astronomy & Astrophysics, 652
Astronomy & Astrophysics, 652, 1-22
Astronomy & Astrophysics, 652, pp. 1-22
Astronomy & Astrophysics, 652
Astronomy & Astrophysics, 652, 1-22
Astronomy & Astrophysics, 652, pp. 1-22
Context. Eta Carinae is a highly eccentric, massive binary system (semimajor axis ~15.5 au) with powerful stellar winds and a phase-dependent wind-wind collision (WWC) zone. The primary star, η Car A, is a luminous blue variable (LBV); the secondary
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d06daaf6607db2ea8e3aee0292014bdb
https://dare.uva.nl/personal/pure/en/publications/vltimatisse-chromatic-aperturesynthesis-imaging-of--carinaes-stellar-wind-across-the-br-line(1b2ef33d-ecf6-411a-8241-108b7aa6f984).html
https://dare.uva.nl/personal/pure/en/publications/vltimatisse-chromatic-aperturesynthesis-imaging-of--carinaes-stellar-wind-across-the-br-line(1b2ef33d-ecf6-411a-8241-108b7aa6f984).html
Publikováno v:
Advances in Astronomy, Vol 2014 (2014)
An overview is presented of the recent advances in understanding the B[e] phenomenon among blue supergiant stars in light of high-angular resolution observations and with an emphasis on the results obtained by means of long baseline optical stellar i
Externí odkaz:
https://doaj.org/article/953c9744743247bd84d787ba9bcccf70
Context. The rarity and deeply embedded nature of young massive stars has limited the understanding of the formation of stars with masses larger than 8 M⊙. Previous work has shown that complementing spectral energy distributions with interferometri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::001517cec019eb78593c575766bc7467
https://lirias.kuleuven.be/handle/123456789/675117
https://lirias.kuleuven.be/handle/123456789/675117