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molecules:extragalactic:hf_extragalactic [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:extragalactic:hf_extragalactic [2019/10/22 13:34] (current) – mueller | ||
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The //J// = 1 – 0 transition was observed in emission with the SPIRE instrument of the // | The //J// = 1 – 0 transition was observed in emission with the SPIRE instrument of the // | ||
P. P. van der Werf, K. G. Isaak, R. Meijerink, et al.,\\ | P. P. van der Werf, K. G. Isaak, R. Meijerink, et al.,\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
The account is sparse, but a detail of the spectrum (van der Werf, private communication) clearly shows the line well-separated from a near-by water line. | The account is sparse, but a detail of the spectrum (van der Werf, private communication) clearly shows the line well-separated from a near-by water line. | ||
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The same transition was seen with the same instrument in absorption toward the ULIRG Arp 220 by\\ | The same transition was seen with the same instrument in absorption toward the ULIRG Arp 220 by\\ | ||
N. Rangwala, P. R. Maloney, J. Glenn, et al.,\\ | N. Rangwala, P. R. Maloney, J. Glenn, et al.,\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
// | // | ||
R. R. Monje, T. G. Phillips, R. Peng, D. C. Lis, D. A. Neufeld, and M. Emprechtinger\\ | R. R. Monje, T. G. Phillips, R. Peng, D. C. Lis, D. A. Neufeld, and M. Emprechtinger\\ | ||
reported on the\\ | reported on the\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
// | // | ||
employing the CSO. Again, the //J// = 1 – 0 transition was observed in absorption. | employing the CSO. Again, the //J// = 1 – 0 transition was observed in absorption. | ||
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Contributor(s): | Contributor(s): | ||
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