The illumination of the GGD 30 nebulosity
| Autor: | N. B. Foley, T. M. Gledhill, R. D. Wolstencroft, S. M. Scarrott |
|---|---|
| Rok vydání: | 1993 |
| Předmět: |
Physics
Reflection nebula Star formation Astronomy Astronomy and Astrophysics Optical polarization Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics Polarization (waves) Mathematics::Geometric Topology Interstellar medium Knot (unit) Space and Planetary Science Astrophysics::Solar and Stellar Astrophysics Astrophysics::Earth and Planetary Astrophysics Herbig–Haro object Emission spectrum Astrophysics::Galaxy Astrophysics |
| Zdroj: | Monthly Notices of the Royal Astronomical Society. 262:175-178 |
| ISSN: | 1365-2966 0035-8711 |
| DOI: | 10.1093/mnras/262.1.175 |
| Popis: | An optical polarization map of the GGD 30 nebulosity shows that, although it shares many of the morphological characteristics of classical cometary nebulae such as NGC 2261/R.Mon, it differs in that the star-like knot at its head is not the illluminating and exciting source as previously assumed. The knot is reflection nebulosity and the true source, completely hidden from direct view at optical wave-lengths, is located some 6 arcsec east of the knot |
| Databáze: | OpenAIRE |
| Externí odkaz: |
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