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Icarus, ISSN 0019-1035, 01/2017, Volume 281, pp. 281 - 285
We have derived homopause temperatures of 180–250 K for the 8-µm north-polar hot spot (8NPHS) of Jupiter by fitting CH emission models to 3 and 8 µm spectra of... 
Aurora | Spectroscopy | Jupiter | Infrared | Atmosphere
Journal Article
Astrophysical Journal, ISSN 0004-637X, 10/2005, Volume 632, Issue 2 I, pp. 882 - 893
Journal Article
Icarus, ISSN 0019-1035, 01/2017, Volume 281, pp. 281 - 285
We have derived homopause temperatures of 180–250 K for the 8-µm north-polar hot spot (8NPHS) of Jupiter by fitting CH emission models to 3 and 8 µm spectra of... 
Aurora | Spectroscopy | Jupiter | Infrared | Atmosphere
Journal Article
Icarus, ISSN 0019-1035, 01/2017, Volume 281, p. 281
We have derived homopause temperatures of 180-250K for the 8-[micro]m north-polar hot spot (8NPHS) of Jupiter by fitting CH.sub.4 emission models to 3 and... 
Analysis | Astronomy | Research institutes | Precipitation (Meteorology)
Journal Article
Icarus, ISSN 0019-1035, 09/2015, Volume 257, pp. 217 - 220
We have obtained 3.3-3.4-μm spectro-images of Jupiter including CH 4 and H 3 + emission lines from both polar regions at the Gemini North telescope. We find... 
Spectroscopy | Jupiter | Aurorae | Atmospheres, composition | Infrared observations
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 12/2007, Volume 671, Issue 2, pp. 1736 - 1747
Journal Article
Icarus, ISSN 0019-1035, 09/2015, Volume 257, p. 217
* New high-resolution (R [approximately equal to]15,000) spectro-images of Jupiter's polar regions at 3.3[mu]m. * The 3-[mu]m CH.sub.4 northern bright spot is... 
Journal Article
Proceedings of the International Astronomical Union, ISSN 1743-9213, 2015, Volume 12, Issue S316, pp. 161 - 162
AbstractWe investigate the formation of young massive clusters near the nuclei in NGC 6946, IC 342, Maffei II, and NGC 7714, using ground-based mid-infrared... 
Infrared | Nearby Galaxies | Star Clusters | Astrophysics | Infrared imaging systems | Star & galaxy formation | Stars & galaxies
Journal Article
Astrophysics and Space Science Proceedings, ISSN 1570-6591, 2013, Volume 37, pp. 159 - 172
Conference Proceeding
ICARUS, ISSN 0019-1035, 01/2017, Volume 281, pp. 281 - 285
We have derived homopause temperatures of 180-250 K for the 8-mu m north-polar hot spot (8NPHS) of Jupiter by fitting CH4 emission models to 3 and 8 mu m... 
Spectroscopy | CASSINI | Infrared | UPPER-ATMOSPHERE | Aurora | BRIGHTENINGS | Jupiter | WAVES | Atmosphere | ASTRONOMY & ASTROPHYSICS | REGIONS | CHEMISTRY | STRATOSPHERE | EMISSION | Spectral emissivity | Emission | Equatorial regions | Particle precipitation | Mixing ratios | Hot spots
Journal Article
Journal Article
Astrophysical Journal, ISSN 0004-637X, 05/2018, Volume 858, Issue 2, p. 97
The coldest brown dwarf, WISE 0855, is the closest known planetary-mass, free-floating object and has a temperature nearly as cold as the solar system gas... 
stars: atmospheres | planets and satellites: atmospheres | brown dwarfs | planets and satellites: gaseous planets | EXTRASOLAR GIANT PLANETS | T-DWARFS | LIGHT CURVES | MODEL | THEORETICAL SPECTRA | DUST | ATMOSPHERIC PROPERTIES | CLOUDS | ASTRONOMY & ASTROPHYSICS | THERMAL STRUCTURE | CHEMISTRY | Physics - Earth and Planetary Astrophysics
Journal Article
Nature, ISSN 0028-0836, 04/2003, Volume 422, Issue 6931, pp. 500 - 502
The H3+ molecular ion plays a fundamental role in interstellar chemistry, as it initiates a network of chemical reactions that produce many molecules. In dense... 
Journal Article
NATURE, ISSN 0028-0836, 04/2003, Volume 422, Issue 6931, pp. 500 - 502
The H-3(+) molecular ion plays a fundamental role in interstellar chemistry, as it initiates a network of chemical reactions that produce many molecules(1,2).... 
DESTRUCTION | DIFFUSE INTERSTELLAR-MEDIUM | DISSOCIATIVE RECOMBINATION | SPECTROSCOPY | ELECTRONS | CLOUDS | MULTIDISCIPLINARY SCIENCES | IONS | MOLECULES
Journal Article
The Journal of Physical Chemistry A, ISSN 1089-5639, 10/2013, Volume 117, Issue 39, pp. 9305 - 9307
Journal Article
Publications of the Astronomical Society of Japan, ISSN 0004-6264, 04/2011, Volume 63, Issue 2, pp. L13 - L17
We present a follow-up observation on Geballe and Oka (2010, ApJ, 709, L70), who found high column densities of H-3(+) similar to 100 pc apart from the... 
Clouds- ISM | Galaxy | Molecules | Center-ISM | Lines and bands- ISM | ISM: lines and bands | H2O | ISM: molecules | ASTRONOMY & ASTROPHYSICS | STARS | OH | ISM: clouds | INTERSTELLAR-MEDIUM | Galaxy: center | SAGITTARIUS
Journal Article
Science, ISSN 0036-8075, 04/2003, Volume 300, Issue 5619, pp. 628 - 630
The smoggy stratosphere of Saturn's largest moon, Titan, veils its surface from view, except at narrow wavelengths centered at 0.83, 0.94, 1.07, 1.28, 1.58,... 
JOVIAN PLANETS | SPECTROPHOTOMETRY | AEROSOLS | METHANE | CARBON-MONOXIDE | IMAGES | CLOUDS | MULTIDISCIPLINARY SCIENCES | 5 MU-M | SPECTRUM | ATMOSPHERE | Methane | Water | Saturn | Carbon Monoxide | Organic Chemicals | Atmosphere | Ice | Extraterrestrial Environment | Stratosphere | Chemical oceanography | Saturn (Planet) | Research | Titan (Satellite) | Planets
Journal Article
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