molecules:ism:aceton

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molecules:ism:aceton [2019/02/25 22:38] – external edit 127.0.0.1molecules:ism:aceton [2019/04/24 16:19] mueller
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 15 years later, this detection was confirmed:\\ 15 years later, this detection was confirmed:\\
 L. E. Snyder, F. J. Lovas, D. M. Mehringer, N. Y. Miao, Y.-J. Kuan, J. M. Hollis, and P. R. Jewell,\\ L. E. Snyder, F. J. Lovas, D. M. Mehringer, N. Y. Miao, Y.-J. Kuan, J. M. Hollis, and P. R. Jewell,\\
-**[[http://dx.doi.org/10.1086/342273|Confirmation of Interstellar Acetone]]**\\+**[[https://doi.org/10.1086/342273|Confirmation of Interstellar Acetone]]**\\
 //Astrophys. J.// **578**, 245–255 (2002).\\ //Astrophys. J.// **578**, 245–255 (2002).\\
  
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 More recently, propanone was detected towards the high-mass star-forming region Orion KL:\\ More recently, propanone was detected towards the high-mass star-forming region Orion KL:\\
 D. N. Friedel, L. E. Snyder, A. J. Remijan, and B. E. Turner,\\ D. N. Friedel, L. E. Snyder, A. J. Remijan, and B. E. Turner,\\
-**[[http://dx.doi.org/10.1086/497986|Detection of Interstellar Acetone toward the Orion-KL Hot Core]]**\\+**[[https://doi.org/10.1086/497986|Detection of Interstellar Acetone toward the Orion-KL Hot Core]]**\\
 //Astrophys. J.// **632**, L95–L98 (2005).\\ //Astrophys. J.// **632**, L95–L98 (2005).\\
 Besides a very large number of transitions in its ground vibrational state, a few lines of the first excited torsional state were reported. Even though the number of vibrationally excited lines is small, the consistent global modeling ensures this aspect of the detection. Besides a very large number of transitions in its ground vibrational state, a few lines of the first excited torsional state were reported. Even though the number of vibrationally excited lines is small, the consistent global modeling ensures this aspect of the detection.
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 J. M. Lykke, A. Coutens, J. K. Jørgensen, M. H. D. van der Wiel, R. T. Garrod, H. S. P. Müller, P. Bjerkeli, T. L. Bourke, H. Calcutt, M. N. Drozdovskaya, C. Favre, E. C. Fayolle, S. K. Jacobsen, K. I. Öberg, M. V. Persson, E. F. van Dishoeck, and S. F. Wampfler\\ J. M. Lykke, A. Coutens, J. K. Jørgensen, M. H. D. van der Wiel, R. T. Garrod, H. S. P. Müller, P. Bjerkeli, T. L. Bourke, H. Calcutt, M. N. Drozdovskaya, C. Favre, E. C. Fayolle, S. K. Jacobsen, K. I. Öberg, M. V. Persson, E. F. van Dishoeck, and S. F. Wampfler\\
 reported on\\ reported on\\
-**[[http://dx.doi.org/10.1051/0004-6361/201629180|The ALMA-PILS Survey: First Detections of Ethylene Oxide, Acetone and Propanal toward the Low-mass Protostar IRAS 16293–2422]]**\\+**[[https://doi.org/10.1051/0004-6361/201629180|The ALMA-PILS Survey: First Detections of Ethylene Oxide, Acetone and Propanal toward the Low-mass Protostar IRAS 16293–2422]]**\\
 //Astrophys. J.// **597**, Art. No. A53 (2017).\\ //Astrophys. J.// **597**, Art. No. A53 (2017).\\
 This report is the first one on the detection of acetone around a low-mass protostar. The Protostellar Interferometric Line Survey (PILS) was carried out with ALMA in its Band 7 (329 – 363 GHz). A total of 186 lines were assigned to acetone. This report is the first one on the detection of acetone around a low-mass protostar. The Protostellar Interferometric Line Survey (PILS) was carried out with ALMA in its Band 7 (329 – 363 GHz). A total of 186 lines were assigned to acetone.
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