2016/05/19 by C. Vastel, Charlotte Vastel, Cecilia Ceccarelli +5 · 1 citation
Physics and Astronomy · #Abundance (ecology) #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Carbon fibers #Core (optical fiber) #Desorption #Emission spectrum #Line (geometry) #Spectral line #Stellar, planetary, and galactic studies #astro-ph.GA
paper · pdf · doi:10.1051/0004-6361/201628427
To appear in A&A Letters
openalex publication_date 2016/05/19 · arxiv created 2016/05/26 · arxiv updated 2016/05/27 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
The L1544 prestellar core has been observed as part of the ASAI IRAM Large Program at 3 mm. These observations led to the detection of many complex molecules. In this Letter, we report the detection of two lines, at 85.5 GHz (40,4–30,3) and 106.9 GHz (50,5–40,4), respectively, of the protonated carbon dioxide ion, HOCO+. We also report the tentative detection of the line at 100.4 GHz (50,5–40,4) of DOCO+. The non-LTE analysis of the detected lines shows that the HOCO+ emission originates in the external layer where non-thermal desorption of other species has previously been observed. Its abundance is (5 ± 2) × 10-11. Modelling of the chemistry involved in the formation and destruction of HOCO+ provides a gaseous CO2 abundance of 2 × 10-7 (with respect to H2) with an upper limit of 2 × 10-6.