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 | 
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