WB89 520: A Small Isolated High Mass Star Forming Region Associated with an Extremely Metal-poor Nebula
2001 ◽
Vol 205
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pp. 284-285
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In this paper, by discussing and analyzing the observational results of near infrared imaging, optical spectroscopy and 12CO molecular line, together with IRAS and NVSS data, we conclude that WB89 520 is an UC HII region with a very young compact stellar cluster. The spectrum of the UC HII region shows that it is an extremely metal-poor nebula, which has the lowest line ratio of [NII]/Hα (∼ 1/56) discovered in the nebulae of our Galaxy until now. We give two possible explanations for the low metallicity.
2018 ◽
Vol 14
(A30)
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pp. 102-102
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Nitrogen and hydrogen fractionation in high-mass star-forming cores from observations of HCN and HNC
2018 ◽
Vol 609
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pp. A129
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2020 ◽
Vol 497
(4)
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pp. 5454-5472
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2012 ◽
Vol 8
(S292)
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pp. 50-50
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2017 ◽
Vol 13
(S336)
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pp. 289-290
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