Optical spectroscopy of the radio pulsar PSR B0656+14
Abstract
We have obtained the spectrum of a middle-aged PSR B0656+14 in the 4300-9000 Å range with the ESO/VLT/FORS2. Preliminary results show that at 4600-7000 Å the spectrum is almost featureless and flat with a spectral index α ν ≃-0.2 that undergoes a change to a positive value at longer wavelengths. Combining with available multiwavelength data suggests two wide, red and blue, flux depressions whose frequency ratio is about 2 and which could be the 1st and 2nd harmonics of electron/positron cyclotron absorption formed at magnetic fields ∼108 G in upper magnetosphere of the pulsar. © Springer Science+Business Media B.V. 2007.
Más información
Título según WOS: | Optical spectroscopy of the radio pulsar PSR B0656+14 |
Título según SCOPUS: | Optical spectroscopy of the radio pulsar PSR B0656+14 |
Título de la Revista: | ASTROPHYSICS AND SPACE SCIENCE |
Volumen: | 308 |
Número: | 01-abr |
Editorial: | Springer |
Fecha de publicación: | 2007 |
Página de inicio: | 545 |
Página final: | 549 |
Idioma: | English |
URL: | http://www.scopus.com/inward/record.url?eid=2-s2.0-34248200408&partnerID=q2rCbXpz |
DOI: |
10.1007/s10509-007-9308-z |
Notas: | ISI, SCOPUS |