The nature of the extended blue continuum in Cygnus A

التفاصيل البيبلوغرافية
العنوان: The nature of the extended blue continuum in Cygnus A
المؤلفون: Martin Shaw, Clive Tadhunter
المصدر: Monthly Notices of the Royal Astronomical Society. 267:589-604
بيانات النشر: Oxford University Press (OUP), 1994.
سنة النشر: 1994
مصطلحات موضوعية: Physics, Wavelength, Stellar population, Space and Planetary Science, Continuum (design consultancy), Extinction (astronomy), Astronomy, Astronomy and Astrophysics, Astrophysics, Cygnus A, Spatial distribution, Spectral line, Galaxy
الوصف: We have used long-slit spectra to derive spatial continuum profiles at UV, optical and near-IR wavelengths in the central region of Cygnus A. The line-free continuum colour distributions derived from these are used to identify the spatial distribution of, and relative contribution from, the featureless blue continuum (FBC) in each of the principal nuclear subcomponents in this object. The FBC is spatially extended, covering a region ∼4-4.5 arcsec in extent along a P.A. of 105°. Beyond this, the emission is predominantly that of the old stellar population in the underlying galaxy. In addition, the core region is markedly redder than the adjacent NW and SE nuclear subcomponents, suggesting considerable reddening/extinction
تدمد: 1365-2966
0035-8711
الوصول الحر: https://explore.openaire.eu/search/publication?articleId=doi_________::a2ce3a7cc2096617be34a5291aa8248eTest
https://doi.org/10.1093/mnras/267.3.589Test
حقوق: OPEN
رقم الانضمام: edsair.doi...........a2ce3a7cc2096617be34a5291aa8248e
قاعدة البيانات: OpenAIRE