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  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
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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