TY - JOUR
T1 - Visible, near-infrared and mid-infrared spectra of solid O2at 6-33 K
AU - Lo, Jen Iu
AU - Lu, Hsiao Chi
AU - Hung, Wei Hsiu
AU - Ogilvie, J. F.
AU - Cheng, Bing Ming
N1 - Publisher Copyright:
© 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.
PY - 2022/8/1
Y1 - 2022/8/1
N2 - We report spectra in the visible and near-infrared wavelength range 350-1155 nm and in the mid-infrared range 500-5000 cm-1 (2-20 μm) of molecular oxygen at temperatures 6-33 K. In mid-infrared spectra, a sharp line at 1552.4 cm-1 was observed at a deposition temperature of 6 K. The intensity, profile and position of this feature depended sensitively upon the deposition temperature as a result of a connection with lattice imperfections; instead, a triplet feature at 1545.7, 1548.1 and 1549.6 cm-1 appeared at temperatures 9 and 12 K, but disappeared at 18, 24 and 30 K. Additional infrared lines of solid α-O2 were observed at 1591 and 1617 cm-1, which exhibited a reversible behaviour through the α-β phase transition temperature at 24 K. The transmissions of solid O2 showed nearly no change in wavenumber range 500-2000 cm-1 (5-20 μm) at temperatures 6-33 K; above 2000 cm-1 (<5 μm), the transmission of solid O2 depended strongly on temperature. Roughly, the transmission of solid O2 at temperatures 6-21 K fluctuated slightly in the visible and near-infrared region, whereas it decreased greatly at 24 K and continuously diminished further at higher temperatures. Notably, a broad absorption of solid β-O2 was observed in the wavelength region 350-700 nm at temperatures 27, 30 and 33 K.
AB - We report spectra in the visible and near-infrared wavelength range 350-1155 nm and in the mid-infrared range 500-5000 cm-1 (2-20 μm) of molecular oxygen at temperatures 6-33 K. In mid-infrared spectra, a sharp line at 1552.4 cm-1 was observed at a deposition temperature of 6 K. The intensity, profile and position of this feature depended sensitively upon the deposition temperature as a result of a connection with lattice imperfections; instead, a triplet feature at 1545.7, 1548.1 and 1549.6 cm-1 appeared at temperatures 9 and 12 K, but disappeared at 18, 24 and 30 K. Additional infrared lines of solid α-O2 were observed at 1591 and 1617 cm-1, which exhibited a reversible behaviour through the α-β phase transition temperature at 24 K. The transmissions of solid O2 showed nearly no change in wavenumber range 500-2000 cm-1 (5-20 μm) at temperatures 6-33 K; above 2000 cm-1 (<5 μm), the transmission of solid O2 depended strongly on temperature. Roughly, the transmission of solid O2 at temperatures 6-21 K fluctuated slightly in the visible and near-infrared region, whereas it decreased greatly at 24 K and continuously diminished further at higher temperatures. Notably, a broad absorption of solid β-O2 was observed in the wavelength region 350-700 nm at temperatures 27, 30 and 33 K.
KW - ISM: molecules
KW - Infrared: ISM
KW - Methods: laboratory: molecular
KW - Molecular data
KW - Ultraviolet: ISM
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U2 - 10.1093/mnras/stac1524
DO - 10.1093/mnras/stac1524
M3 - Article
AN - SCOPUS:85133689025
SN - 0035-8711
VL - 514
SP - 2815
EP - 2820
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 2
ER -