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cloister Wrote:
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> Clearly, they don't know
>
> "Here we report the first observation of a
> large-scale (∼0.26 pc) HH jet driven by a
> candidate proto-brown dwarf. This jet has
> been designated the HH number HH 1165. The
> driving source of the jet is a very low-luminosity
> Class I object, Mayrit 1701117 (hereafter
> M1701117), which lies at the cusp of the
> stellar/sub-stellar boundary and will
> likely evolve
> into a brown dwarf. HH 1165 shows many of the
> characteristics of a large-scale jet including
> multiple knots, bow-shocks, a C-shaped morphology
> and a reflection nebula. The first hints
> of a jet driven by M1701117 were seen in moderate
> resolution spectra presented in Riaz
> et al. (2015). Follow-up UV-Visual Echelle
> Spectrometer (UVES) spectra provided more
> information on the jet close to the driving
> source. Images taken with SOAR have revealed
> the spectacular nature of the jet. In this paper,
> we present both the SOAR and UVES
> data. While the jet is not extended in the UVES
> data, much can still be learnt from the
> various accretion and outflow associated
> spectral line diagnostics"
>
>
> Whereas these people do
>
> [www.youtube.com]
Lol. The idiot Thornhill and his clueless EU acolytes! Where has the clown written his stuff up?
-------------------------------------------------------
> Clearly, they don't know
>
> "Here we report the first observation of a
> large-scale (∼0.26 pc) HH jet driven by a
> candidate proto-brown dwarf. This jet has
> been designated the HH number HH 1165. The
> driving source of the jet is a very low-luminosity
> Class I object, Mayrit 1701117 (hereafter
> M1701117), which lies at the cusp of the
> stellar/sub-stellar boundary and will
> likely evolve
> into a brown dwarf. HH 1165 shows many of the
> characteristics of a large-scale jet including
> multiple knots, bow-shocks, a C-shaped morphology
> and a reflection nebula. The first hints
> of a jet driven by M1701117 were seen in moderate
> resolution spectra presented in Riaz
> et al. (2015). Follow-up UV-Visual Echelle
> Spectrometer (UVES) spectra provided more
> information on the jet close to the driving
> source. Images taken with SOAR have revealed
> the spectacular nature of the jet. In this paper,
> we present both the SOAR and UVES
> data. While the jet is not extended in the UVES
> data, much can still be learnt from the
> various accretion and outflow associated
> spectral line diagnostics"
>
>
> Whereas these people do
>
> [www.youtube.com]
Lol. The idiot Thornhill and his clueless EU acolytes! Where has the clown written his stuff up?
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