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

Natale Robba; null Fiorentino; null Monelli; null Burderi; null D'Antona; null Testa; Fabio D'Antona

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

Natale Robba, Fiorentino, Monelli, Burderi, D'Antona, Testa, Fabio D'Antona

Fisica e Chimica - Emilio Segrè

Risultato della ricerca: Other › peer review

1 Citazioni (Scopus)

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
Pagine	565-568
Numero di pagine	4
Stato di pubblicazione	Published - 2005

All Science Journal Classification (ASJC) codes

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title = "Optical counterpart of the XTE J0929-314 in quiescence: constraints on the magnetic field",

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. {\textcopyright} 2005 American Institute of Physics.",

author = "Natale Robba and Fiorentino and Monelli and Burderi and D'Antona and Testa and Fabio D'Antona",

year = "2005",

language = "English",

pages = "565--568",

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TY - CONF

T1 - Optical counterpart of the XTE J0929-314 in quiescence: constraints on the magnetic field

AU - Robba, Natale

AU - Fiorentino, null

AU - Monelli, null

AU - Burderi, null

AU - D'Antona, null

AU - Testa, null

AU - D'Antona, Fabio

PY - 2005

Y1 - 2005

N2 - 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.

AB - 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.

UR - http://hdl.handle.net/10447/12268

UR - https://aip.scitation.org/doi/pdf/10.1063/1.2130286?class=pdf

M3 - Other

SP - 565

EP - 568

ER -