Chemical evolution of the HC3N and N2H+ molecules in dense cores of the Vela C giant molecular cloud complex

We have observed the HC3N(J = 10–9) and N2H+ (J = 1–0) lines toward the Vela C molecular clouds with the Mopra 22 m telescope to study the chemical characteristics of dense cores. The intensity distributions of these molecules are similar to each other at an angular resolution of 53″, corresponding...

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Veröffentlicht in:	Publications of the Astronomical Society of Japan 2016-02, Vol.68 (1)
Hauptverfasser:	Ohashi, Satoshi, Tatematsu, Ken'ichi, Fujii, Kosuke, Sanhueza, Patricio, Nguyen Luong, Quang, Choi, Minho, Hirota, Tomoya, Mizuno, Norikazu
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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