Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/33206
Title: | Science case study and scientific simulations for the enhanced X-ray Timing Polarimetry mission, eXTP | Authors: | DE ROSA, Alessandra BURGIO,G.F. DI SALVO,T. DRAGO,A. LA PLACA, RICCARDO SERAFINELLI, ROBERTO GAMBINO,A. GUALTIERI,L. MASELLI, Alessandro FEROCI, MARCO STELLA, Luigi BOMBACI,I. BURDERI,L. CAMPANA, Sergio CAPITANIO, FIAMMA CASELLA, Piergiorgio D'AI', Antonino D'AMMANDO, FILIPPO DE MARTINO, Domitilla EVANGELISTA, YURI FERRARI,V. NARDINI, Emanuele ORLANDINI, MAURO PACCIANI, LUIGI PAGLIARA,G. PANI,P. RIGGIO,A. RODRIGUEZ CASTILLO, Guillermo Andres SANNA,A. Schulze,H.J. TAVERNA,R. Tombesi, Francesco VERCELLONE, STEFANO |
Issue Date: | 2022 | Journal: | MEMORIE DELLA SOCIETA ASTRONOMICA ITALIANA | Number: | 93 | Issue: | 2 | First Page: | 245 | Abstract: | The X-ray astronomy mission eXTP (enhanced X-ray Timing Polarimetry) is designed to study matter under extreme conditions of density, gravity and magnetism. Primary goals are the determination of the equation of state (EoS) of matter at supranuclear density, the physics in extremely strong magnetic fields, the study of accretion in strong-field gravity (SFG) regime. Primary targets include isolated and binary neutron stars, strong magneticfield systems like magnetars, and stellar-mass and supermassive black holes. In this paper we report about key observations and simulations with eXTP on the primary objectives involving accretion under SFG regimes and determination of NS-EoS | URI: | http://hdl.handle.net/20.500.12386/33206 | URL: | https://memsait.oa-roma.inaf.it/wp-content/uploads/2022/11/2022MmSAI..2-3..245D.pdf http://sait.oat.ts.astro.it/ToC.htm |
ISSN: | 0037-8720 | Bibcode ADS: | 2022MmSAI..93b.245D | Fulltext: | open |
Appears in Collections: | 1.01 Articoli in rivista |
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2022MmSAI..2-3..245D.pdf | Pdf editoriale | 573.76 kB | Adobe PDF | View/Open |
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