We present VLT observations of the optical counterpart of th X-ray millisecond pulsar XTE J0929-314 in quiescence. We detected a very faint candidate in agreement with the position given by radio and X observation. From the observed optical flux we inferred un upper limit to the magnetic field of the system. © 2005 American Institute of Physics.

MONELLI M, FIORENTINO G, BURDERI L, DANTONA F, ROBBA NR, TESTA V (2005). Optical counterpart of the XTE J0929-314 in quiescence: constraints on the magnetic field. In aaa (pp.565-568) [10.1063/1.2130286].

Optical counterpart of the XTE J0929-314 in quiescence: constraints on the magnetic field

D'ANTONA, Fabio;ROBBA, Natale;
2005-01-01

Abstract

We present VLT observations of the optical counterpart of th X-ray millisecond pulsar XTE J0929-314 in quiescence. We detected a very faint candidate in agreement with the position given by radio and X observation. From the observed optical flux we inferred un upper limit to the magnetic field of the system. © 2005 American Institute of Physics.
Interacting Binaries: Accretion, Evolution & Outcomes
Cefalù; Sicilia
July 4-10 2004
2005
4
https://aip.scitation.org/doi/pdf/10.1063/1.2130286?class=pdf
Published by AIP Conference Proceedings, eds. L. Burderi, L. A. Antonelli, F. D'Antona, T. Di Salvo, G.L. Israel, L. Piersanti, O. Straniero, A. Tornambe.
MONELLI M, FIORENTINO G, BURDERI L, DANTONA F, ROBBA NR, TESTA V (2005). Optical counterpart of the XTE J0929-314 in quiescence: constraints on the magnetic field. In aaa (pp.565-568) [10.1063/1.2130286].
Proceedings (atti dei congressi)
MONELLI M; FIORENTINO G; BURDERI L; DANTONA F; ROBBA NR; TESTA V
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10447/12268
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