R. Fuentetaja, M. Ag'undez, C. Cabezas, B. Tercero, N. Marcelino, J. R. Pardo, P. D. Vicente, J. Cernicharo
{"title":"通过 QUIJOTE 线测量发现 TMC-1 中的 HCCCH_2CCH","authors":"R. Fuentetaja, M. Ag'undez, C. Cabezas, B. Tercero, N. Marcelino, J. R. Pardo, P. D. Vicente, J. Cernicharo","doi":"10.1051/0004-6361/202348777","DOIUrl":null,"url":null,"abstract":"We present the first detection in space of 1,4-pentadiyne. It has\nbeen found towards TMC-1 with the QUIJOTE line survey in the 31-50 GHz range. \nWe observed a total of 17 transitions with $J$ = 2 up to 13 and $K_a$ = \n0,1 and 2. The observed transitions allowed us to derive a rotational temperature \nof 9.5 pm 0.5 K and a column density of (5.0 pm 0.5)times 1012 cm$^ $. \nThis molecule was the last non-cyclic isomer of the C$_5$H$_4$ family that could be detected via radio astronomy. A computational chemistry study was performed to determine the energies of the five most stable isomers. The isomer ($c$-C$_3$H$_3$CCH) has a considerably higher energy than the \nothers, and it has not yet been detected.\nTo better understand the chemical reactions involving these species, \nwe compared the ethynyl and cyano derivatives. The observed \nabundances of these species are in good agreement with the branching ratios of \nthe formation reactions studied with our chemical model of TMC-1.","PeriodicalId":505693,"journal":{"name":"Astronomy & Astrophysics","volume":"31 7","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-07-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Discovery of HCCCH_2CCH in TMC-1 with the QUIJOTE line survey\",\"authors\":\"R. Fuentetaja, M. Ag'undez, C. Cabezas, B. Tercero, N. Marcelino, J. R. Pardo, P. D. Vicente, J. Cernicharo\",\"doi\":\"10.1051/0004-6361/202348777\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We present the first detection in space of 1,4-pentadiyne. It has\\nbeen found towards TMC-1 with the QUIJOTE line survey in the 31-50 GHz range. \\nWe observed a total of 17 transitions with $J$ = 2 up to 13 and $K_a$ = \\n0,1 and 2. The observed transitions allowed us to derive a rotational temperature \\nof 9.5 pm 0.5 K and a column density of (5.0 pm 0.5)times 1012 cm$^ $. \\nThis molecule was the last non-cyclic isomer of the C$_5$H$_4$ family that could be detected via radio astronomy. A computational chemistry study was performed to determine the energies of the five most stable isomers. The isomer ($c$-C$_3$H$_3$CCH) has a considerably higher energy than the \\nothers, and it has not yet been detected.\\nTo better understand the chemical reactions involving these species, \\nwe compared the ethynyl and cyano derivatives. The observed \\nabundances of these species are in good agreement with the branching ratios of \\nthe formation reactions studied with our chemical model of TMC-1.\",\"PeriodicalId\":505693,\"journal\":{\"name\":\"Astronomy & Astrophysics\",\"volume\":\"31 7\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-07-09\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Astronomy & Astrophysics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1051/0004-6361/202348777\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomy & Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1051/0004-6361/202348777","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Discovery of HCCCH_2CCH in TMC-1 with the QUIJOTE line survey
We present the first detection in space of 1,4-pentadiyne. It has
been found towards TMC-1 with the QUIJOTE line survey in the 31-50 GHz range.
We observed a total of 17 transitions with $J$ = 2 up to 13 and $K_a$ =
0,1 and 2. The observed transitions allowed us to derive a rotational temperature
of 9.5 pm 0.5 K and a column density of (5.0 pm 0.5)times 1012 cm$^ $.
This molecule was the last non-cyclic isomer of the C$_5$H$_4$ family that could be detected via radio astronomy. A computational chemistry study was performed to determine the energies of the five most stable isomers. The isomer ($c$-C$_3$H$_3$CCH) has a considerably higher energy than the
others, and it has not yet been detected.
To better understand the chemical reactions involving these species,
we compared the ethynyl and cyano derivatives. The observed
abundances of these species are in good agreement with the branching ratios of
the formation reactions studied with our chemical model of TMC-1.