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THE IDENTIFICATION OF PROBABLE SiS EMISSION AT 13-14 μm IN SPECTRA OF GALACTIC S STARS

  • Published:2011-02-16 Issue:2 Volume:729 Page:121
  • ISSN:0004-637X
  • Container-title:The Astrophysical Journal
  • language:
  • Short-container-title:ApJ

Author:

Sloan G. C.,Hony S.,Smolders K.,Decin L.,Zijlstra A. A.,Feast M. W.,van Wyk F.,van Loon J. Th.,Groenewegen M. A. T.,Sahai R.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 7 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Spectroscopy and molecule opacity investigation on excited states of SiS;Chinese Physics B;2024-04-01

2. Transition properties of five lowest–lying singlet and three lowest–lying triplet states of silicon monosulphide molecule;Journal of Quantitative Spectroscopy and Radiative Transfer;2021-09

3. The 21 μm and 30 μm emission features in carbon-rich objects;Astrophysics and Space Science;2020-05

4. Spitzerinfrared spectrograph point source classification in the Small Magellanic Cloud;Monthly Notices of the Royal Astronomical Society;2015-06-25

5. Catalytic conversion of acetylene to polycyclic aromatic hydrocarbons over particles of pyroxene and alumina;Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences;2013-07-13
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