Píldoras con AthenaPequeñas reseñas sobre temas científicos y tecnológicos de la misión Athena con el objetivo de acercar su ciencia y desarrollo tecnológico, no sólo a la comunidad científica sino también a los no expertos. Buscar #AthenaNuggets 22: Athena and the Square Kilometer Array joining forces to detect the most rarefied gas in the Universe 02 Mar 2018 Franco Vazza1, Stefano Ettori2 & Chiara Ferrari3(1) Università di Bologna,Universität Hamburg(2) Osservatorio di Astrofisica... Leer más + #AthenaNuggets 21: Balancing on the Edge: Detecting X-rays with Transition Edge Sensors 01 Feb 2018 Simon Bandler (NASA/GSFC), on behalf of the team developing the X-IFU X-ray microcalorimeter arrays.At the core of... Leer más + #AthenaNuggets 20: Unveiling the Hot, High Redshift Universe with the Athena WFI 06 Ene 2018 Steven Allen & Adam Mantz, Stanford UniversityStudies of galaxy groups and galaxy clusters, the largest objects in the Universe... Leer más + #AthenaNuggets 19: Athena End-to-End Simulations 05 Ene 2018 J. Wilms1 (ECAP), P. Peille2 (CNES), T. Dauser1 (ECAP) & E. Cucchetti3 (IRAP)(1)... Leer más + #AthenaNuggets 19: Accretion and Ejection Around Black Holes: the Disc-Jet Connection 30 Nov 2017 Chris Done, Center for Extragalactic Astronomy, Department of Physics, University of DurhamBlack holes are black, but material captured by... Leer más + #AthenaNuggets 17: Observing Bright Sources with the Athena-WFI 02 Nov 2017 Jörn Wilms1, Thomas Dauser1 and Arne Rau2(1)Remeis Observatory & ECAP, Universität Erlangen-Nürnberg (2)Max-Planck Institut fuer... Leer más + #AthenaNuggets 16: Ultra-Luminous X-Ray Sources: When Compact Objects Become Gluttonous Accretors 05 Oct 2017 Christian Motch. Observatoire Astronomique StrasbourgGalaxies often host non-nuclear accreting ultra-luminous X-ray sources (ULXs). Leer más + #AthenaNuggets 15: Athena Instrument Background 27 Sep 2017 Simone Lotti1 & Silvano Molendi2 (1) INAF/IAPS(2) INAF/IASFObservations of faint X-ray sources are traditionally limited by instrumental background. Leer más + #AthenaNuggets 14: How are winds generated around stellar-mass black holes and neutron stars? 31 Ago 2017 María Díaz-Trigo, ESOThe brightest X-ray sources in our galaxy are X-ray binaries. In these systems, a normal star and... Leer más + Paginación Primera página « Página anterior ‹‹ Page 1 Page 2 Page 3 Page 4 Page 5 Página actual 6 Page 7 Page 8 Siguiente página ›› Última página »
#AthenaNuggets 22: Athena and the Square Kilometer Array joining forces to detect the most rarefied gas in the Universe 02 Mar 2018 Franco Vazza1, Stefano Ettori2 & Chiara Ferrari3(1) Università di Bologna,Universität Hamburg(2) Osservatorio di Astrofisica... Leer más +
#AthenaNuggets 21: Balancing on the Edge: Detecting X-rays with Transition Edge Sensors 01 Feb 2018 Simon Bandler (NASA/GSFC), on behalf of the team developing the X-IFU X-ray microcalorimeter arrays.At the core of... Leer más +
#AthenaNuggets 20: Unveiling the Hot, High Redshift Universe with the Athena WFI 06 Ene 2018 Steven Allen & Adam Mantz, Stanford UniversityStudies of galaxy groups and galaxy clusters, the largest objects in the Universe... Leer más +
#AthenaNuggets 19: Athena End-to-End Simulations 05 Ene 2018 J. Wilms1 (ECAP), P. Peille2 (CNES), T. Dauser1 (ECAP) & E. Cucchetti3 (IRAP)(1)... Leer más +
#AthenaNuggets 19: Accretion and Ejection Around Black Holes: the Disc-Jet Connection 30 Nov 2017 Chris Done, Center for Extragalactic Astronomy, Department of Physics, University of DurhamBlack holes are black, but material captured by... Leer más +
#AthenaNuggets 17: Observing Bright Sources with the Athena-WFI 02 Nov 2017 Jörn Wilms1, Thomas Dauser1 and Arne Rau2(1)Remeis Observatory & ECAP, Universität Erlangen-Nürnberg (2)Max-Planck Institut fuer... Leer más +
#AthenaNuggets 16: Ultra-Luminous X-Ray Sources: When Compact Objects Become Gluttonous Accretors 05 Oct 2017 Christian Motch. Observatoire Astronomique StrasbourgGalaxies often host non-nuclear accreting ultra-luminous X-ray sources (ULXs). Leer más +
#AthenaNuggets 15: Athena Instrument Background 27 Sep 2017 Simone Lotti1 & Silvano Molendi2 (1) INAF/IAPS(2) INAF/IASFObservations of faint X-ray sources are traditionally limited by instrumental background. Leer más +
#AthenaNuggets 14: How are winds generated around stellar-mass black holes and neutron stars? 31 Ago 2017 María Díaz-Trigo, ESOThe brightest X-ray sources in our galaxy are X-ray binaries. In these systems, a normal star and... Leer más +