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molecules:ism:pn [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:pn [2019/10/18 12:54] (current) – mueller | ||
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B. E. Turner and J. Bally\\ | B. E. Turner and J. Bally\\ | ||
reported on the\\ | reported on the\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
The //J// = 2 – 1, 3 – 2, and 5 –& | The //J// = 2 – 1, 3 – 2, and 5 –& | ||
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L. M. Ziurys, S. N. Milam, A. J. Apponi, and N. J. Woolf\\ | L. M. Ziurys, S. N. Milam, A. J. Apponi, and N. J. Woolf\\ | ||
reported on\\ | reported on\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Nature// **447**, 1094–1097 (2007).\\ | //Nature// **447**, 1094–1097 (2007).\\ | ||
PN was identified in the course of a molecular line survey with the ARO 12 m and the SMT 10 m telescopes, covering large sections of the 75–270 GHz region. | PN was identified in the course of a molecular line survey with the ARO 12 m and the SMT 10 m telescopes, covering large sections of the 75–270 GHz region. | ||
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S. N. Milam, D. T. Halfen, E. D. Tenenbaum, A. J. Apponi, N. J. Woolf, and L. M. Ziurys\\ | S. N. Milam, D. T. Halfen, E. D. Tenenbaum, A. J. Apponi, N. J. Woolf, and L. M. Ziurys\\ | ||
reported on\\ | reported on\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
// | // | ||
Several lines of PN were detected with the same instruments as above toward the envelopes of the carbon-rich late-type stars V1610 Cygni (aka CRL 2688) and CW Leonis (aka IRC +10216). | Several lines of PN were detected with the same instruments as above toward the envelopes of the carbon-rich late-type stars V1610 Cygni (aka CRL 2688) and CW Leonis (aka IRC +10216). | ||
PN was also detected around a (low-mass) class 0 proto-star: | PN was also detected around a (low-mass) class 0 proto-star: | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
by T. Yamaguchi, S. Takano, N. Sakai, T. Sakai, S.-Y. Liu, Y.-N. Su, N. Hirano, S. Takakuwa, Y. Aikawa, H. Nomura, and S. Yamamoto,\\ | by T. Yamaguchi, S. Takano, N. Sakai, T. Sakai, S.-Y. Liu, Y.-N. Su, N. Hirano, S. Takakuwa, Y. Aikawa, H. Nomura, and S. Yamamoto,\\ | ||
//Publ. Astron. Soc. Japan// **63**, L37–L41 (2011).\\ | //Publ. Astron. Soc. Japan// **63**, L37–L41 (2011).\\ |