TEMPORAL PROPERTIES OF GX 301−2 OVER A YEAR-LONG OBSERVATION WITH SuperAGILE
Y. Evangelista,M. Feroci,E. Costa,E. Del Monte,I. Donnarumma,I. Lapshov,F. Lazzarotto,L. Pacciani,M. Rapisarda,P. Soffitta,A. Argan,G. Barbiellini,F. Boffelli,A. Bulgarelli,P. Caraveo,P. W. Cattaneo,A. Chen,F. D'Ammando,G. Di Cocco,F. Fuschino,M. Galli,F. Gianotti,A. Giuliani,C. Labanti,P. Lipari,F. Longo,M. Marisaldi,S. Mereghetti,E. Moretti,A. Morselli,A. Pellizzoni,F. Perotti,G. Piano,P. Picozza,M. Pilia,M. Prest,G. Pucella,A. Rappoldi,S. Sabatini,E. Striani,M. Tavani,M. Trifoglio,A. Trois,E. Vallazza,S. Vercellone,V. Vittorini,A. Zambra,L. A. Antonelli,S. Cutini,C. Pittori,B. Preger,P. Santolamazza,F. Verrecchia,P. Giommi,L. Salotti ASTROPHYSICAL JOURNAL(2010)
Key words
pulsars: individual (GX 3012),stars: neutron,X-rays: binaries
AI Read Science
Must-Reading Tree
Example

Generate MRT to find the research sequence of this paper