Millimeter wave spectrum and search for vinyl isocyanate toward Sgr B2(N) with ALMA

Context. The interstellar detections of isocyanic acid (HNCO), methyl isocyanate (CH 3 NCO), and very recently also ethyl isocyanate (C 2 H 5 NCO) invite the question of whether or not vinyl isocyanate (C 2 H 3 NCO) can be detected in the interstellar medium. There are only low-frequency spectroscop...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2022-10, Vol.666, p.A50
Hauptverfasser: Vávra, K., Kolesniková, L., Belloche, A., Garrod, R. T., Koucký, J., Uhlíková, T., Luková, K., Guillemin, J.-C., Kania, P., Müller, H. S. P., Menten, K. M., Urban, Š.
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Sprache:eng
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Zusammenfassung:Context. The interstellar detections of isocyanic acid (HNCO), methyl isocyanate (CH 3 NCO), and very recently also ethyl isocyanate (C 2 H 5 NCO) invite the question of whether or not vinyl isocyanate (C 2 H 3 NCO) can be detected in the interstellar medium. There are only low-frequency spectroscopic data (
ISSN:0004-6361
1432-0746
1432-0756
DOI:10.1051/0004-6361/202243627