Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]Infrared and optical polarimetric observations of the quasar 3C 345 are presented, which show a decrease in the degree of polarization with frequency previously observed by Smith et al., and interpreted by them as the result of dilution of the polarized flux by a non-polarized thermal component (the "blue bump"). The new data are compared to previous fits of this model to 3C 345, and the validity of the model is discussed.Peer reviewe
International audienceContext: Spectropolarimetry of AGNs is a powerful tool for studying the struct...
Abstract. New linear polarization measurements (mainly in the V band) are presented for 203 quasi-st...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
Original article can be found at: http://www.adsabs.harvard.edu/ Copyright European Southern Observa...
Original paper can be found at: http://161.58.115.79/pubs/cs/222-252.html--Copyright Astronomical So...
The near-infrared shape of the big blue bump component in quasar spectra has been essentially unknow...
International audienceIf the disappearance of the broad emission lines observed in changing-look qua...
International audienceA handful of active galactic nuclei (AGN) have shown strong spectral variation...
Original article can be found at: www3.interscience.wiley.com Copyright Blackwell Publishing / Royal...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
© 2022. The Author(s). Published by the American Astronomical Society. This work is licenced under t...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
Polarization is a basic property of light and is fundamentally linked to the internal geometry of a ...
International audienceContext: Spectropolarimetry of AGNs is a powerful tool for studying the struct...
Abstract. New linear polarization measurements (mainly in the V band) are presented for 203 quasi-st...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
Original article can be found at: http://www.adsabs.harvard.edu/ Copyright European Southern Observa...
Original paper can be found at: http://161.58.115.79/pubs/cs/222-252.html--Copyright Astronomical So...
The near-infrared shape of the big blue bump component in quasar spectra has been essentially unknow...
International audienceIf the disappearance of the broad emission lines observed in changing-look qua...
International audienceA handful of active galactic nuclei (AGN) have shown strong spectral variation...
Original article can be found at: www3.interscience.wiley.com Copyright Blackwell Publishing / Royal...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
© 2022. The Author(s). Published by the American Astronomical Society. This work is licenced under t...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
Polarization is a basic property of light and is fundamentally linked to the internal geometry of a ...
International audienceContext: Spectropolarimetry of AGNs is a powerful tool for studying the struct...
Abstract. New linear polarization measurements (mainly in the V band) are presented for 203 quasi-st...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...