A SEARCH FOR O-2 IN CO-DEPLETED MOLECULAR CLOUD CORES WITH HERSCHEL

作者：Wirstrom Eva S^*; Charnley Steven B; Cordiner Martin A; Ceccarelli Cecilia

来源：Astrophysical Journal, 2016, 830(2): 102.

DOI：10.3847/0004-637X/830/2/102

• astrochemistry
• ISM: abundances
• ISM: clouds
• ISM: molecules
• molecular processes

The general lack of molecular oxygen in molecular clouds is an outstanding problem in astrochemistry. Extensive searches with the Submillimeter Astronomical Satellite, Odin,. and Herschel have only produced two detections; upper limits to the O-2 abundance in the remaining sources observed are about 1000 times lower than predicted by chemical models. Previous atomic oxygen observations and inferences from observations of other molecules indicated that high abundances of O atoms might be present in dense cores exhibiting large amounts of CO depletion. Theoretical arguments concerning the oxygen gas-grain interaction in cold dense cores suggested that, if O atoms could survive in the gas after most of the rest of the heavy molecular material has frozen out onto dust, then O-2 could be formed efficiently in the gas. Using Herschel HIFI, we searched a small sample of four depletion cores-L1544, L694-2, L429, and. Oph D-for emission in the low excitation O-2 N-J = 3(3)-1(2) line at 487.249 GHz. Molecular oxygen was not detected and we derive upper limits to its abundance in the range of N(O-2)/N(H-2) approximate to (0.6-1.6) x 10(-7). We discuss the absence of O-2 in the light of recent laboratory and observational studies.

• 出版日期2016-10-20