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Herschel Planetary Nebula Survey (HerPlaNS): hydrogen recombination laser lines in Mz 3

Autor: E. Mendoza, Alexander G. G. M. Tielens, Zulema Abraham, Masaaki Otsuka, K. Exter, M. L. Leal-Ferreira, Rodolfo Montez, J. Lepine, Albert A. Zijlstra, Samuel Walton, Eva Villaver, Pedro P. B. Beaklini, Peter A. M. van Hoof, Isabel Aleman, Toshiya Ueta

Publikováno v: Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 477(4), 4499-4510
Aleman, I, Exter, K, Ueta, T, Walton, S, Tielens, A G G M, Zijlstra, A, Montez, R, Abraham, Z, Otsuka, M, Beaklini, P P B, van Hoof, P A M, Villaver, E, Leal-Ferreira, M L, Mendoza, E & Lepine, J D R 2018, ' Herschel Planetary Nebula Survey (HerPlaNS): Hydrogen Recombination Laser Lines in Mz 3 ', Royal Astronomical Society. Monthly Notices, vol. 477, no. 4, pp. 4499-4510 . https://doi.org/10.1093/mnras/sty966

The bipolar nebula Menzel 3 (Mz 3) was observed as part of the \textit{Herschel} Planetary Nebula Survey (\textit{HerPlaNS}), which used the PACS and SPIRE instruments aboard the \textit{Herschel Space Observatory} to study a sample of planetary nebu

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::11af4af66c65062531a576c848c1290b
https://hdl.handle.net/1887/69937

Mass ratio from Doppler beaming and Rømer delay versus ellipsoidal modulation in the Kepler data of KOI-74★

Autor: Robin Lombaert, K. Exter, Chris M. Copperwheat, T. R. Marsh, Elmé Breedt, Yves Fremat, R. H. Østensen, Gert Raskin, Péter Pápics, Herman Hensberge, S. Prins, Alain Jorissen, Boris T. Gänsicke, Pieter Degroote, Detlev Koester, S. Van Eck, Wim Pessemier, S. Pyrzas, H. Van Winckel, Conny Aerts, Steven Bloemen

Publikováno v: Monthly Notices of the Royal Astronomical Society. 422:2600-2608

We present a light curve analysis and radial velocity study of KOI-74, an eclipsing A star + white dwarf binary with a 5.2 day orbit. Aside from new spectroscopy covering the orbit of the system, we used 212 days of publicly available Kepler observat

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::ece7cc78f3ffe60e8873351c5322daf9
https://doi.org/10.1111/j.1365-2966.2012.20818.x

3D Spectroscopy of Herbig-Haro Objects

Autor: Sebastián F. Sánchez, Robert Estalella, Angels Riera, K. Exter, Begoña García-Lorenzo, Roberto López, Gerard Gómez

Publikováno v: Eso Astrophysics Symposia ISBN: 9783540734901

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::348bbc9de4602faf3df1ad87b23e39f9
https://doi.org/10.1007/978-3-540-73491-8_56

The orbits of subdwarf B + main-sequence binaries

Autor: R. H. Østensen, Pieter Degroote, Gert Raskin, J. Vos, Steven Bloemen, K. Smolders, P. De Cat, P. Neyskens, Elizabeth M. Green, Thomas Masseron, H. Van Winckel, Andrew Tkachenko, Ulrich Heber, Bram Acke, K. Exter, Thomas Rauch, Ellen Ringat, J. Menu, Robin Lombaert, Patricia Lampens, K. De Smedt

Publikováno v: Astronomy & Astrophysics. 548:A6

The predicted orbital period histogram of an sdB population is bimodal with a peak at short (< 10 days) and long (> 250 days) periods. Observationally, there are many short-period sdB systems known, but only very few long-period sdB binaries are iden

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d6b5490e59047e5cef018c9feb6c3da7
https://doi.org/10.1051/0004-6361/201219723