Zobrazeno 1 - 10
of 15
pro vyhledávání: '"C. van Kerckhoven"'
Autor:
S. Hony, Louis J. Allamandola, Aggm Tielens, Els Peeters, C. van Kerckhoven, B. van Diedenhoven, Douglas M. Hudgins
Publikováno v:
Astrophysical Journal, 611(2), 928-939. IOP PUBLISHING LTD
We present spectra of the 3.3 mum and 11.2 mum polycyclic aromatic hydrocarbon (PAH) features of a large number of stellar sources, planetary nebulae, reflection nebulae, H II regions, and galaxies, obtained with Infrared Space Observatory Short Wave
Autor:
Aggm Tielens, Els Peeters, Louis J. Allamandola, C. van Kerckhoven, Douglas M. Hudgins, S. Hony, Charles W. Bauschlicher
Publikováno v:
Astronomy & Astrophysics, 390, 1089-1113. EDP Sciences
IR spectroscopy provides a valuable tool for the characterisation and identification of interstellar molecular species. Here, we present 6-9 mum spectra of a sample of reflection nebulae, HII regions, YSOs, evolved stars and galaxies that show strong
Publikováno v:
Symposium - International Astronomical Union. 197:349-362
ISO has shown that the mid–IR spectra of almost all sources are dominated by narrow emission features collectively known as the UIR bands. These bands are carried by a family of polycyclic aromatic hydrocarbon molecules containing about 50 C-atoms.
Autor:
Thomas Henning, C. Boersma, Fred Lahuis, Jeroen Bouwman, Alexander G. G. M. Tielens, L. B. F. M. Waters, C. van Kerckhoven
Publikováno v:
Astronomy & Astrophysics, 484(1), 241-249. EDP Sciences
Astronomy & astrophysics, 484(1), 241-249. EDP Sciences
Astronomy & astrophysics, 484(1), 241-249. EDP Sciences
Context. Infrared ( IR) spectra provide a prime tool to study the characteristics of polycyclic aromatic hydrocarbon ( PAH) molecules in regions of star formation. Herbig Ae/Be stars are a class of young pre-main sequence stellar objects of intermedi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c806ba5139013b38d0e95e13613265e7
http://arxiv.org/abs/0804.1199
http://arxiv.org/abs/0804.1199
Autor:
J. Daszynska-Daskiewicz, Karolien Lefever, C. van Kerckhoven, Richard Scuflaire, Conny Aerts, Pieter Deroo, Katrien Kolenberg, Maryline Briquet, L. Le Guillou, Tijl Verhoelst, T. Maas, Greet Decin, J. Vanautgaerden, K. Reyniers, Anwesh Mazumdar, Gert Raskin, C. Barban, Marc-Antoine Dupret, E. Broeders, E. Vanhollebeke, Kadri Yakut, H. Van Winckel, K. Goossens, W. De Meester, G. Davignon, Bart Vandenbussche, J. Cuypers, P. De Cat, Bram Acke, C. Waelkens, Jonas Debosscher, Leen Decin, R. Van Malderen, K. Uytterhoeven, Maarten Reyniers, S. De Ruyter, R. Drummond, M. Ausseloos, S. Saesen, J. De Ridder
Publikováno v:
Astronomy & Astrophysics, 463, 243-249
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2007, 463, pp.243-249. ⟨10.1051/0004-6361:20066202⟩
Astronomy & Astrophysics, 463, 1, pp. 243-249
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2007, 463, pp.243-249. ⟨10.1051/0004-6361:20066202⟩
Astronomy & Astrophysics, 463, 1, pp. 243-249
Contains fulltext : 34555.pdf (Publisher’s version ) (Open Access) Aims. We selected a large sample of O-B stars that were considered as (candidate) slowly pulsating B, beta Cep, and Maia stars after the analysis of their hipparcos data. We analyse
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ddca2a32a5b253eeaa5c854a6f1d8f6
https://lirias.kuleuven.be/handle/123456789/250715
https://lirias.kuleuven.be/handle/123456789/250715
Publikováno v:
Astronomy & astrophysics, 384(2), 568-584. EDP Sciences
We present an analysis of ISO-SWS observations of the Herbig Ae/Be stars HD 97048 and Elias 1. Besides the well-known family of IR emission bands at 3.3, 6.2, "7.7", 8.6 and 11.2 mum these objects show strong, peculiar emission features at 3.43 and 3
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bfb276a806c8694205e11ebb9f8eea9d
https://research.rug.nl/en/publications/5642ea14-f072-4506-918d-43f9ff11bdee
https://research.rug.nl/en/publications/5642ea14-f072-4506-918d-43f9ff11bdee
Autor:
Sacha Hony, D. M. Hudgins, C. van Kerckhoven, Els Peeters, Alexander G. G. M. Tielens, L. J. Allamandola
Publikováno v:
Astronomy & Astrophysics, 370, 1030-1043. EDP Sciences
Astronomy & astrophysics, 370(3), 1030-1043. EDP Sciences
Astronomy & astrophysics, 370(3), 1030-1043. EDP Sciences
We present 10-15 micron spectra of a sample of H II regions, YSOs and evolved stars that show strong unidentified infrared emission features, obtained with the ISO/SWS spectrograph on-board ISO. These spectra reveal a plethora of emission features wi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4a82759408eb7c394debdbfeffc7587d
https://dare.uva.nl/personal/pure/en/publications/the-ch-outofplane-bending-modes-of-pah-molecules-in-astrophysical-environments(f6fc9045-f094-455b-8c02-568de40915e2).html
https://dare.uva.nl/personal/pure/en/publications/the-ch-outofplane-bending-modes-of-pah-molecules-in-astrophysical-environments(f6fc9045-f094-455b-8c02-568de40915e2).html
Autor:
Gert Raskin, G. Davignon, T. Reyniers, J. Daszyńska-Daszkiewicz, J. De Ridder, K. Uytterhoeven, Maarten Reyniers, S. De Ruyter, L. Decin, M. Ausseloos, E. Broeders, P. De Cat, T. Maas, Greet Decin, C. Schoenaers, C. Waelkens, J. Cuypers, J. Vanautgaerden, W. De Meester, C. van Kerckhoven, Conny Aerts, H. Van Winckel, R. Van Malderen, Bram Acke, Katrien Kolenberg, Bart Vandenbussche
Publikováno v:
NASA Astrophysics Data System
We report on the first results from observations of 28 variable B stars obtained with the new Mercator telescope (La Palma). Besides confirming the pulsational nature of known and candidate β Cephei and slowly pulsating B stars, we also present new
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::69b9781ef02c6cd77cffd5222c902ef2
https://ui.adsabs.harvard.edu/#abs/2004ASPC..310..238D
https://ui.adsabs.harvard.edu/#abs/2004ASPC..310..238D
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