Detection of a Noble Gas Molecular Ion, 36ArH+, in the Crab Nebula

被引:146
作者
Barlow, M. J. [1 ]
Swinyard, B. M. [1 ,2 ]
Owen, P. J. [1 ]
Cernicharo, J. [3 ]
Gomez, H. L. [4 ]
Ivison, R. J. [5 ]
Krause, O. [6 ]
Lim, T. L. [2 ]
Matsuura, M. [1 ]
Miller, S. [1 ]
Olofsson, G. [7 ]
Polehampton, E. T. [2 ,8 ]
机构
[1] Univ London Univ Coll, Dept Phys & Astron, London WC1E 6BT, England
[2] Rutherford Appleton Lab, Space Sci & Technol Dept, Didcot OX11 0QX, Oxon, England
[3] CSIC, Inst Nacl Tecn Aeroesp, Lab Mol Astrophys, Dept Astrophys,Ctr Astrobiol, Madrid 28850, Spain
[4] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales
[5] Royal Observ Edinburgh, UK Astron Technol Ctr, Edinburgh EH9 3HJ, Midlothian, Scotland
[6] Max Planck Inst Astron, D-69117 Heidelberg, Germany
[7] Stockholm Univ, AlbaNova Univ Ctr, Dept Astron, S-10691 Stockholm, Sweden
[8] Univ Lethbridge, Dept Phys & Astron, Inst Space Imaging Sci, Lethbridge, AB T1K 3M4, Canada
关键词
ROTATIONAL-EXCITATION; HERSCHEL; SPECTROSCOPY; KNOTS; HEH+;
D O I
10.1126/science.1243582
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
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- and 1234.6-gigahertz J = 1-0 and 2-1 rotational lines of (ArH+)-Ar-36 at several positions in the Crab Nebula, a supernova remnant known to contain both molecular hydrogen and regions of enhanced ionized argon emission. Argon-36 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 (ArH+)-Ar-36 emission lines is electron collisions in partially ionized regions with electron densities of a few hundred per centimeter cubed.
引用
收藏
页码:1343 / 1345
页数:3
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