Zobrazeno 1 - 10
of 133
pro vyhledávání: '"Bowman DM"'
Autor:
Shenar, T, Sana, H, Marchant, P, Pablo, B, Richardson, N, Moffat, AFJ, Van Reeth, T, Barba, RH, Bowman, DM, Broos, P, Crowther, PA, Clark, JS, de Koter, A, de Mink, SE, Dsilva, K, Grafener, G, Howarth, ID, Langer, N, Mahy, L, Apellaniz, J Maiz, Pollock, AMT, Schneider, FRN, Townsley, L, Vink, JS
ispartof: ASTRONOMY & ASTROPHYSICS vol:650 status: published
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1131::ac3ef694cbea0946bbafa3436d60418f
https://lirias.kuleuven.be/handle/123456789/677927
https://lirias.kuleuven.be/handle/123456789/677927
Autor:
Bowman, DM, Aerts, C, Johnston, C, Pedersen, MG, Rogers, TM, Edelmann, PVF, Simon-Diaz, S, Van Reeth, T, Buysschaert, B, Tkachenko, A, Triana, SA
Publikováno v:
Bowman, D M, Aerts, C, Johnston, C, Pedersen, M G, Rogers, T M, Edelmann, P V F, Simon-Diaz, S, Van Reeth, T, Buysschaert, B, Tkachenko, A & Triana, S A 2019, ' Photometric detection of internal gravity waves in upper main-sequence stars ', Astronomy & Astrophysics, vol. 621, 135 . https://doi.org/10.1051/0004-6361/201833662
Astronomy & Astrophysics
Astronomy & Astrophysics
© ESO 2019. Context. Main sequence stars with a convective core are predicted to stochastically excite internal gravity waves (IGWs), which effectively transport angular momentum throughout the stellar interior and explain the observed near-uniform
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::24f82d2c2dd079c197cdc0cea6e5adfc
https://pure.au.dk/portal/da/publications/photometric-detection-of-internal-gravity-waves-in-upper-mainsequence-stars(b94ed696-e2db-4575-a9c4-ec9ef3608388).html
https://pure.au.dk/portal/da/publications/photometric-detection-of-internal-gravity-waves-in-upper-mainsequence-stars(b94ed696-e2db-4575-a9c4-ec9ef3608388).html
Publikováno v:
EPJ Web of Conferences, Vol 101, p 06013 (2015)
The δ Sct star KIC 7106205 showed amplitude modulation in a single p mode, whilst all other p and g modes remained stable in amplitude and phase over 1470 d of the Kepler dataset. The data were divided into 30 time bins of equal length and a series
Autor:
Niemczura, E, Murphy, SJ, Smalley, B, Uytterhoeven, K, Pigulski, A, Lehmann, H, Bowman, DM, Catanzaro, G, van Aarle, E, Bloemen, S, Briquet, M, De Cat, P, Drobek, D, Eyer, L, Gameiro, JFS, Gorlova, N, Kaminski, K, Lampens, P, Marcos-Arenal, P, Papics, PI, Vandenbussche, B, Van Winckel, H, Steslicki, M, Fagas, M
The Kepler space mission provided near-continuous and high-precision photometry of about 207 000 stars, which can be used for asteroseismology. However, for successful seismic modeling it is equally important to have accurate stellar physical paramet
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::c7d61fa780dba8e2de548181643baed2
https://lirias.kuleuven.be/handle/123456789/504885
https://lirias.kuleuven.be/handle/123456789/504885
Publikováno v:
Medical Journal of Australia; 3/21/2011, Vol. 194 Issue 6, p319-322, 4p
Publikováno v:
Journal of Bioethical Inquiry; Mar2009, Vol. 6 Issue 1, p25-36, 12p
Akademický článek
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Akademický článek
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Autor:
Fisher B, Dignam J, Bryant J, DeCillis A, Wickerham DL, Wolmark N, Costantino J, Redmond C, Fisher ER, Bowman DM, Deschênes L, Dimitrov NV, Margolese RG, Robidoux A, Shibata H, Terz J, Paterson AH, Feldman MI, Farrar W, Evans J
Publikováno v:
JNCI: Journal of the National Cancer Institute; 11/6/96, Vol. 88 Issue 21, p1529-1542, 14p
Autor:
Bowman DM
Publikováno v:
Journal of Bioethical Inquiry; Mar2009, Vol. 6 Issue 1, p141-143, 3p