Zobrazeno 1 - 10
of 40
pro vyhledávání: '"Detmers, R.G."'
Autor:
Buchwitz, M., Reuter, M., Schneising, O., Hewson, W., Detmers, R.G., Boesch, H., Hasekamp, O.P., Aben, I., Bovensmann, H., Burrows, J.P., Butz, A., Chevallier, F., Dils, B., Frankenberg, C., Heymann, J., Lichtenberg, G., De Mazière, M., Notholt, J., Parker, R., Warneke, T., Zehner, C., Griffith, D.W.T., Deutscher, N.M., Kuze, A., Suto, H., Wunch, D.
Publikováno v:
In Remote Sensing of Environment 15 December 2017 203:276-295
Active Galactic Nuclei (AGN) are accreting supermassive black holes at the centers of galaxies. They can have a profound impact on the evolution of their host galaxies and surroundings by means of their outflows of ionized gas. However we still lack
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::d1818d066f44522c65ca2722c6bebad4
https://dspace.library.uu.nl/handle/1874/214870
https://dspace.library.uu.nl/handle/1874/214870
Autor:
Ness, J.-U., Osborne, J.P., Dobrotka, A., Page, K.L., Drake, J.J., Pinto, C., Detmers, R.G., Schwarz, G., Bode, M.F., Beardmore, A.P., Starrfield, S., Hernanz, M., Sala, G., Krautter, J., Woodward, C.E.
Two XMM-Newton observations of the fast classical nova V2491 Cyg were carried out in short succession on days 39.93 and 49.62 after discovery, during the supersoft source (SSS) phase, yielding simultaneous X-ray and UV light curves and high-resolutio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______101::a55c884b7bb3669c8f5cea1a0e665ac2
https://dspace.library.uu.nl/handle/1874/210656
https://dspace.library.uu.nl/handle/1874/210656
We analyzed three XMM-Newton observations of the Seyfert 1 galaxy Mrk 509, with the goal of detecting small variations in the ionized outflow properties. Measurements such as these are limited by the quality of the cross-calibration between RGS, the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______101::9c320973a14eeb303b238042a4e14bcf
https://dspace.library.uu.nl/handle/1874/202801
https://dspace.library.uu.nl/handle/1874/202801
Autor:
Detmers, R.G., Kaastra, J.S., McHardy, I.M., Astrophysics, Sub High energy Astrophysics begr 1/1/15, Dep Natuurkunde
Publikováno v:
Astronomy and Astrophysics, 504(2), 409. EDP Sciences
We study the long time scale variability of the gas responsible for the X-ray narrow emission lines in the Seyfert 1 galaxy NGC 5548, in order to constrain the location and geometry of the emitting gas. Using X-ray spectra taken with the Chandra−LE
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::a821dc9275a8d321b078df1a385c269b
https://dspace.library.uu.nl/handle/1874/43557
https://dspace.library.uu.nl/handle/1874/43557
Autor:
Detmers, R.G., Kaastra, J.S., Costantini, E., McHardy, I.M., Verbunt, F.W.M., Astrophysics, Sub High energy Astrophysics begr 1/1/15, Dep Natuurkunde
Publikováno v:
Astronomy and Astrophysics, 488(1), 67. EDP Sciences
We study the variability of the warm absorber and the gas responsible for the emission lines in the Seyfert 1 galaxy NGC 5548 to constrain the location and physical properties of these components. Using X-ray spectra acquired using the Chandra-LETGS
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::6e502843cbe9306a530c9dc906bb156b
https://dspace.library.uu.nl/handle/1874/32394
https://dspace.library.uu.nl/handle/1874/32394
Autor:
Detmers, R.G., Langer, N., Podsiadlowski, Ph., Izzard, R.G., Astrophysics, Sub High energy Astrophysics begr 1/1/15, Afd Astrophysics begr 1/1/17, Dep Natuurkunde
Publikováno v:
Astronomy and Astrophysics, 484(3), 831. EDP Sciences
Context. The collapsar model requires rapidly rotating Wolf-Rayet stars as progenitors of long gamma-ray bursts. However, Galactic Wolf-Rayet stars rapidly lose angular momentum due to their intense stellar winds. Aims. We investigate whether the tid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::37f7cb54bedf6871376466c570232e35
https://dspace.library.uu.nl/handle/1874/32393
https://dspace.library.uu.nl/handle/1874/32393
Autor:
Toledano, O., Moreno, E., Koenigsberger, G., Detmers, R.G., Langer, N., Astrophysics, Sub High energy Astrophysics begr 1/1/15, Afd Astrophysics begr 1/1/17
Publikováno v:
Astronomy and Astrophysics, 461(3), 1057. EDP Sciences
Context. Stellar oscillations are excited in non-synchronously rotating stars in binary systems due to the tidal forces. Tangential components of the tides can drive a shear flow which behaves as a differentially forced rotating structure in a strati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::d49ae1dc1dd3483f6e43e406c719a8ef
https://dspace.library.uu.nl/handle/1874/41711
https://dspace.library.uu.nl/handle/1874/41711
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Akademický článek
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