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The Astrophysical Journal Letters, ISSN 1538-4357, 07/2003, Volume 592, Issue 1, pp. L13 - L16
Previous optical studies found an unexpected deficit of bars at z > 0.7. To investigate the effects of band shifting, we have studied the fraction of barred... 
Galaxies: evolution | Cosmology: observations | Galaxies: formation | Infrared: galaxies | galaxies : evolution | EVOLUTION | galaxies : formation | SPIRAL GALAXIES | ASTRONOMY & ASTROPHYSICS | cosmology : observations | infrared : galaxies | BARS | MORPHOLOGY
Journal Article
Astrophysical Journal, ISSN 0004-637X, 12/2014, Volume 796, Issue 2
We report interferometric imaging of [CII] and OH emission toward the center of the galaxy protocluster associated with the z=5.3 submillimeter galaxy (SMG)... 
galaxies: formation | radio lines: galaxies | galaxies: starburst | cosmology: observations | galaxies: active | galaxies: high-redshift
Journal Article
Astrophysical Journal, ISSN 0004-637X, 02/2014, Volume 796, Issue 2, pp. 1 - 14
We report interferometric imaging of [CII] ( super(2)P sub(3/2) arrow right super(2)P sub(1/2)) and OH ( super(2)[Pi] sub(1/2) J = 3/2 arrow right 1/2)... 
Spirals | Dwarf galaxies | Imaging | Continuums | Spectral energy distribution | Emission | Disks | Arrays | Density
Journal Article
The Astrophysical Journal Supplement Series, ISSN 1538-4365, 08/2015, Volume 219, Issue 2, p. 22
Journal Article
Astrophysical Journal, Supplement Series, ISSN 0067-0049, 12/2011, Volume 197, Issue 2, pp. jQuery1323919395755='48' - jQuery1323919395755='48'
Journal Article
Astrophysical Journal, Supplement Series, ISSN 0067-0049, 08/2015, Volume 219, Issue 2, pp. 1 - 20
Journal Article
The Astrophysical Journal, ISSN 1538-4357, 11/2016, Volume 832, Issue 2, p. 151
Journal Article
The Astrophysical Journal, ISSN 1538-4357, 11/2014, Volume 796, Issue 2, p. 84
We report interferometric imaging of [C II]({sup 2} P {sub 3/2}→{sup 2} P {sub 1/2}) and OH({sup 2}Π{sub 1/2} J = 3/2→1/2) emission toward the center of the... 
RED SHIFT | DISTANCE | TRIPLETS | DUSTS | ENERGY SPECTRA | DENSITY | COSMOLOGY | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | METALS | MASS | STARS | GALAXIES | EMISSION | RADIATION PRESSURE | UNIVERSE
Journal Article
Astrophysical Journal, ISSN 0004-637X, 07/2013, Volume 772, Issue 1
The H II region luminosity function (LF) is an important tool for deriving the birthrates and mass distribution of OB associations and is an excellent tracer... 
LUMINOSITY | TELESCOPES | SPATIAL RESOLUTION | MASS DISTRIBUTION | PHOTONS | SENSITIVITY | STAR CLUSTERS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | SCALING | GALAXIES | EMISSION | GIANT STARS | COSMIC DUST
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 07/2013, Volume 772, Issue 1, p. 27
Journal Article
Astrophysical Journal, ISSN 0004-637X, 07/2013, Volume 772, Issue 1, pp. 1 - 15
The H II region luminosity function (LF) is an important tool for deriving the birthrates and mass distribution of OB associations and is an excellent tracer... 
galaxies: individual | HII regions | HUBBLE-SPACE-TELESCOPE | SPIRAL GALAXIES | HOST GALAXIES | M51 | ZERO-POINT | CIRCUMNUCLEAR STARBURST RING | STAR-FORMATION LAW | H II regions | ASTRONOMY & ASTROPHYSICS | MASS | HII-REGIONS | SIZE DISTRIBUTION | Size distribution | Galaxies | Hubble Space Telescope | Luminosity | Tools | Tracers
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 12/2008, Volume 689, Issue 1, pp. 148 - 152
Spiral arm spurs are prominent features that have been observed in extinction and 8 mu m emission in nearby galaxies. In order to understand their molecular... 
Galaxies:individual (M51, NGC 5194) galaxies:ISM | Stars:formation | Galaxies:spiral ISM:structure | stars: formation | SPIRAL GALAXIES | galaxies: ISM | CLOUDS | ASTRONOMY & ASTROPHYSICS | MASS | STAR-FORMATION | galaxies: individual (M51, NGC5194) | SHOCKS | galaxies: spiral | ISM: structure | INSTABILITIES
Journal Article
Astrophysical Journal, ISSN 0004-637X, 07/2010, Volume 717, Issue 1
We present a study of the average properties of luminous infrared galaxies detected directly at 24 {mu}m in the COSMOS field using a median stacking analysis... 
LUMINOSITY | RED SHIFT | DUSTS | ENERGY SPECTRA | GALACTIC EVOLUTION | FLUX DENSITY | BOLOMETERS | EVOLUTION | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | MEASURING INSTRUMENTS | PHYSICAL PROPERTIES | OPTICAL PROPERTIES | STARS | GALAXIES | SPECTRA | UNIVERSE | GALAXY NUCLEI
Journal Article
Journal Article
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