Open AccessNear‐infrared imaging polarimetry of dusty young stars
Author(s) -
Hales A. S.,
Gledhill T. M.,
Barlow M. J.,
Lowe K. T. E.
Publication year - 2006
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1111/j.1365-2966.2005.09820.x
Subject(s) - physics , polarimetry , polarimeter , stars , astrophysics , polarization (electrochemistry) , infrared , telescope , astronomy , hubble space telescope , radius , infrared telescope , optics , scattering , chemistry , computer security , computer science
We have carried out JHK polarimetric observations of 11 dusty young stars, by using the polarimeter module IRPOL2 with the near‐infrared camera UIST on the 3.8‐m United Kingdom Infrared Telescope (UKIRT). Our sample targeted systems for which UKIRT‐resolvable discs had been predicted by model fits to their spectral energy distributions. Our observations have confirmed the presence of extended polarized emission around TW Hya and around HD 169142. HD 150193 and HD 142666 show the largest polarization values among our sample, but no extended structure was resolved. By combining our observations with Hubble Space Telescope (HST) coronographic data from the literature, we derive the J ‐ and H ‐band intrinsic polarization radial dependences of the disc of TW Hya. We find the polarizing efficiency of the disc is higher at H than at J , and we confirm that the J ‐ and H ‐band percentage polarizations are reasonably constant with radius in the region between 0.9 and 1.3 arcsec from the star. We find that the objects for which we have detected extended polarizations are those for which previous modelling has suggested the presence of flared discs, which are predicted to be brighter than flat discs and thus would be easier to detect polarimetrically.