Herschel spectral-line mapping of the HH211 protostellar system
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چکیده
منابع مشابه
SiO J=5–4 in the HH211 protostellar jet imaged with the SMA
We have mapped the SiO J=5–4 line at 217GHz from the HH2̇11 molecular outflow with the Submillimeter Array (SMA). The high resolution map (1.6×0.9) shows that the SiO J=5–4 emission comes from the central narrow jet along the outflow axis with a width of ∼0.8 (∼ 250AU) FWHM. The SiO jet consists of a chain of knots separated by 3–4 (∼ 1000AU) and most of the SiO knots have counterparts in shocke...
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ژورنال
عنوان ژورنال: Astronomy & Astrophysics
سال: 2018
ISSN: 0004-6361,1432-0746
DOI: 10.1051/0004-6361/201833057