The long-wavelength view of GG Tau A: rocks in the ring world

We present the first detection of GG Tau A at centimetre wavelengths, made with the Arcminute Microkelvin Imager Large Array at a frequency of 16 GHz (λ = 1.8 cm). The source is detected at >6 σrms with an integrated flux density of S 16 GHz = 249 ± 45 μJy. We use these new centimetre-wave data,...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2013-10, Vol.435 (2), p.1139-1146
1. Verfasser:	Scaife, Anna M. M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Dust Markov analysis Mathematical models Monte Carlo simulation Parameter estimation Protoplanetary disks
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