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Images were obtained of the (fluorescent) molecular hydrogen 1-0 S(1) line, and of the 3.3 micron emission feature, in Orion's Bar and three reflection nebulae. The emission from these species appears to come from the same spatial locations in all sources observed. This suggests that the 3.3 micron feature is excited by the same energetic UV-photons which cause the molecular hydrogen to fluoresce
Original paper can be found at: http://astrosociety.org/pubs/cs/195-221.html Copyright ASPObservatio...
Context. Because of its large angular size and proximity to the Milky Way, NGC 253, an archetypal st...
The pure rotational S(2) line of molecular hydrogen at 12.28 microns was looked for in 44 positions ...
This paper presents near-infrared spectroscopy of fluorescent molecular hydrogen (H2) emission from ...
The newly commissioned University of New South Wales Infrared Fabry-Perot (UNSWIRF) has been used to...
We present observations of H_2 fluorescence at wavelengths between 1000 and 1200 A from the bright r...
Using the Infrared Spectrograph on board the Spitzer Space Telescope, we have detected emission in t...
The total shocked and fluorescent molecular hydrogen 1-0 S(1) line luminosities from Orion have been...
Spectra from 1 to 2.5 micron, at 230-430 spectral resolution, are presented of the fluorescent molec...
The 3 micron spectra is presented for the Orion bar region and the Red Rectangle. In both objects sp...
We present near-infrared spectroscopy of fluorescent molecular hydrogen (H_2) emission from molecula...
The central regions of many interacting and early-type spiral galaxies are actively forming stars. T...
Observations of line profiles of the vibrationally excited H2 gas in the Orion molecular cloud are p...
The hydrogen Lyman-α (Lyα) line, a major source of ionization of metals in the circumstellar disks o...
The infrared emission spectrum of H2 excited by ultraviolet absorption, followed by fluorescence, wa...
Original paper can be found at: http://astrosociety.org/pubs/cs/195-221.html Copyright ASPObservatio...
Context. Because of its large angular size and proximity to the Milky Way, NGC 253, an archetypal st...
The pure rotational S(2) line of molecular hydrogen at 12.28 microns was looked for in 44 positions ...
This paper presents near-infrared spectroscopy of fluorescent molecular hydrogen (H2) emission from ...
The newly commissioned University of New South Wales Infrared Fabry-Perot (UNSWIRF) has been used to...
We present observations of H_2 fluorescence at wavelengths between 1000 and 1200 A from the bright r...
Using the Infrared Spectrograph on board the Spitzer Space Telescope, we have detected emission in t...
The total shocked and fluorescent molecular hydrogen 1-0 S(1) line luminosities from Orion have been...
Spectra from 1 to 2.5 micron, at 230-430 spectral resolution, are presented of the fluorescent molec...
The 3 micron spectra is presented for the Orion bar region and the Red Rectangle. In both objects sp...
We present near-infrared spectroscopy of fluorescent molecular hydrogen (H_2) emission from molecula...
The central regions of many interacting and early-type spiral galaxies are actively forming stars. T...
Observations of line profiles of the vibrationally excited H2 gas in the Orion molecular cloud are p...
The hydrogen Lyman-α (Lyα) line, a major source of ionization of metals in the circumstellar disks o...
The infrared emission spectrum of H2 excited by ultraviolet absorption, followed by fluorescence, wa...
Original paper can be found at: http://astrosociety.org/pubs/cs/195-221.html Copyright ASPObservatio...
Context. Because of its large angular size and proximity to the Milky Way, NGC 253, an archetypal st...
The pure rotational S(2) line of molecular hydrogen at 12.28 microns was looked for in 44 positions ...
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