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.
Lingua originale | English |
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Pagine | 565-568 |
Numero di pagine | 4 |
Stato di pubblicazione | Published - 2005 |
All Science Journal Classification (ASJC) codes
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