Zobrazeno 1 - 10
of 206
pro vyhledávání: '"Wilms, Jörn"'
Autor:
Basu-Zych, Antara R., Hornschemeier, Ann E., Haberl, Frank, Vulic, Neven, Wilms, Jorn, Zezas, Andreas, Kovlakas, Konstantinos, Ptak, Andrew, Dauser, Thomas
eROSITA, launched on 13 July 2019, will be completing the first all-sky survey in the soft and medium X-ray band in nearly three decades. This 4-year survey, finishing in late 2023, will present a rich legacy for the entire astrophysics community and
Externí odkaz:
http://arxiv.org/abs/2008.01870
Autor:
Enoto, Teruaki, Sasano, Makoto, Yamada, Shin'ya, Tamagawa, Toru, Makishima, Kazuo, Pottschmidt, Katja, Marcu, Diana, Corbet, Robin H. D., Fuerst, Felix, Wilms, Jorn
The symbiotic X-ray binary 4U 1954+319 is a rare system hosting a peculiar neutron star (NS) and an M-type optical companion. Its ~5.4h NS spin period is the longest among all known accretion-powered pulsars and exhibited large (~7%) fluctuations ove
Externí odkaz:
http://arxiv.org/abs/1404.0134
Autor:
Wilms, Jörn.
Tübingen, University, Diss., 1998.
Erscheinungsjahr an der Haupttitelstelle: 1998. - Gedr. Ausg. im Selbstverl. Jörn Wilms, Tübingen.
Erscheinungsjahr an der Haupttitelstelle: 1998. - Gedr. Ausg. im Selbstverl. Jörn Wilms, Tübingen.
Autor:
Tovmassian, Gagik, Yungelson, Lev, Rauch, Thomas, Suleimanov, Valery, Napiwotzki, Ralf, Stasinska, Grazyna, Tomsick, John, Wilms, Jorn, Morisset, Christophe, Pena, Miriam, Richer, Michael G.
We present a detailed investigation of SBS1150+599A, a close binary star hosted by the planetary nebula PN G135.9+55.9 (TS01, Stasinska et al, 2009). The nebula, located in the Galactic halo, is the most oxygen-poor one known to date and is the only
Externí odkaz:
http://arxiv.org/abs/1003.0639
We present the results of the analysis of the broad-band spectrum of Cygnus X-1 from 3.0 to 200 keV, using data from a 10 ksec observation by the Rossi X-ray Timing Explorer. The spectrum can be well described phenomenologically by an exponentially c
Externí odkaz:
http://arxiv.org/abs/astro-ph/9707322
We apply our self-consistent accretion disk corona (ADC) model, with two different geometries, to the broad-band X-ray spectrum of the black hole candidate Cygnus X-1. As shown in a companion paper (Dove, Wilms, and Begelman), models where the Compto
Externí odkaz:
http://arxiv.org/abs/astro-ph/9705130
We present the properties of accretion disk corona (ADC) models, where the radiation field, the temperature, and the total opacity of the corona are determined self-consistently. We use a non-linear Monte Carlo code to perform the calculations. As an
Externí odkaz:
http://arxiv.org/abs/astro-ph/9705108
Autor:
Madsen, Kristin K., García, Javier A., Stern, Daniel, Amini, Rashied, Basso, Stefano, Coutinho, Diogo, Grefenstette, Brian W., Kenyon, Steven, Moretti, Alberto, Morrissey, Patrick, Nandra, Kirpal, Pareschi, Giovanni, Predehl, Peter, Rau, Arne, Spiga,, Daniele, Wilms, Jörn, Zhang, William W., Marshall, Herman, Rothschild, Richard
Publikováno v:
Frontiers in Astronomy & Space Sciences; 2024, p01-10, 10p
Autor:
Barillier, Erin, Grinberg, Victoria, Horn, David, Nowak, Michael A, Remillard, Ronald A, Steiner, James F, Walton, Dominic J, Wilms, Jörn
4U 1957+11 is a black hole candidate system that has been in a soft X-ray spectral state since its discovery. We present analyses of recent joint NICER and NuSTAR spectra, which are extremely well-described by a highly inclined disk accreting into a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7b9c21a3134f11542b70c63eef702cd5