molecules:extragalactic:hf_extragalactic

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molecules:extragalactic:hf_extragalactic [2019/02/25 22:38] – external edit 127.0.0.1molecules: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 //Herschel// satellite toward the ultra-luminous infrared galaxie (ULIRG) Mrk 231:\\ The //J// = 1 – 0 transition was observed in emission with the SPIRE instrument of the //Herschel// satellite toward the ultra-luminous infrared galaxie (ULIRG) Mrk 231:\\
 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/10.1051/0004-6361/201014682|Black Hole Accretion and Star-Formation as Drivers of Gas Excitation and Chemistry in Markarian 231]]**\\+**[[https://doi.org/10.1051/0004-6361/201014682|Black Hole Accretion and Star-Formation as Drivers of Gas Excitation and Chemistry in Markarian 231]]**\\
 //Astron. Astrophys.// **518**, (2010) Art. No. L42.\\ //Astron. Astrophys.// **518**, (2010) Art. No. L42.\\
 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/10.1088/0004-637X/743/1/94|Observations of Arp 220 Using //Herschel//-SPIRE: An Unprecedented View of the Molecular Gas in an Extreme Star Formation Environment]]**\\+**[[https://doi.org/10.1088/0004-637X/743/1/94|Observations of Arp 220 Using //Herschel//-SPIRE: An Unprecedented View of the Molecular Gas in an Extreme Star Formation Environment]]**\\
 //Astrophys. J.// **743**, (2011) Art. No. 94. //Astrophys. J.// **743**, (2011) Art. No. 94.
  
 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/10.1088/2041-8205/742/2/L21|Discovery of Hydrogen Fluoride in the Cloverleaf Quasar at //z// = 2.56]]**\\+**[[https://doi.org/10.1088/2041-8205/742/2/L21|Discovery of Hydrogen Fluoride in the Cloverleaf Quasar at //z// = 2.56]]**\\
 //Astrophys. J.// **743**, (2011) Art. No. 94;\\ //Astrophys. J.// **743**, (2011) Art. No. 94;\\
 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): H. S. P. Müller; 12, 2010; 04, 2013 Contributor(s): H. S. P. Müller; 12, 2010; 04, 2013
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