2013/12/12 by M. J. Barlow, B. M. Swinyard, P. Owen +11 · 1 citation
Physics and Astronomy · #Astrophysics and Star Formation Studies #Gamma-ray bursts and supernovae #Stellar, planetary, and galactic studies #astro-ph.GA
paper · pdf · doi:10.1126/science.1243582
published as Science, 342, 1343-1345 (2013) · Published in Science on 13th December 2013; 14 pages, 2 figures, 1 table
openalex publication_date 2013/12/12 · arxiv created 2013/12/17 · arxiv updated 2013/12/18 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
Noble gas molecules have not hitherto been detected in space. From spectra obtained with the Herschel Space Observatory, we report the detection of emission in the 617.5 GHz and 1234.6 GHz J = 1-0 and 2-1 rotational lines of 36ArH+ at several positions in the Crab Nebula, a supernova remnant known to contain both H2 molecules and regions of enhanced ionized argon emission. 36Ar is believed to have originated from explosive nucleosynthesis in massive stars during core-collapse supernova events. Its detection in the Crab Nebula, the product of such a supernova event, confirms this expectation. The likely excitation mechanism for the observed 36ArH+ emission lines is electron collisions in partially ionized regions with electron densities of a few hundred per centimeter cubed.