Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2015, Volume 447, Issue 4, pp. 3824 - 3831
Soft X-ray intensity at 0.89 keV along the North Polar Spur (NPS) is shown to follow the extinction law due to the interstellar gas in the Aquila Rift by...
Radio lines: ISM-X-rays: diffuse background | Galaxy: centre | ISM: individual objects: Aquila Rift | ISM: individual objects: North Polar Spur | ISM: kinematics and dynamics | WIND | DISTANCE | CLOUD | LARGE-SCALE | MODEL | BUBBLES | X-rays: diffuse background | radio lines: ISM | NUCLEUS | ASTRONOMY & ASTROPHYSICS | GALACTIC-CENTER | RADIO | HALO | Physics - Astrophysics of Galaxies
Radio lines: ISM-X-rays: diffuse background | Galaxy: centre | ISM: individual objects: Aquila Rift | ISM: individual objects: North Polar Spur | ISM: kinematics and dynamics | WIND | DISTANCE | CLOUD | LARGE-SCALE | MODEL | BUBBLES | X-rays: diffuse background | radio lines: ISM | NUCLEUS | ASTRONOMY & ASTROPHYSICS | GALACTIC-CENTER | RADIO | HALO | Physics - Astrophysics of Galaxies
Journal Article
Astrophysics and Space Science, ISSN 0004-640X, 10/2018, Volume 363, Issue 10, pp. 1 - 6
We present a multi-wavelength correlation study of diffuse ultraviolet radiation using GALEX observations towards the Aquila Rift. Apart from airglow and...
Aquila Rift | Astrophysics and Astroparticles | Astrobiology | Cosmology | Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics) | Diffuse UV background | Excess emission | Physics | Astronomy, Observations and Techniques | GALEX | EVOLUTION | INTERSTELLAR DUST GRAINS | MISSION | ASTRONOMY & ASTROPHYSICS | RADIATION | EXTINCTION | SCATTERING | GALAXY | Analysis | Radiation | Ultraviolet radiation | Correlation | Hydrogen | Correlation analysis | Emission analysis | Optical analysis | Fluorescence | Spectroscopic analysis | Airglow | Physics - Astrophysics of Galaxies
Aquila Rift | Astrophysics and Astroparticles | Astrobiology | Cosmology | Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics) | Diffuse UV background | Excess emission | Physics | Astronomy, Observations and Techniques | GALEX | EVOLUTION | INTERSTELLAR DUST GRAINS | MISSION | ASTRONOMY & ASTROPHYSICS | RADIATION | EXTINCTION | SCATTERING | GALAXY | Analysis | Radiation | Ultraviolet radiation | Correlation | Hydrogen | Correlation analysis | Emission analysis | Optical analysis | Fluorescence | Spectroscopic analysis | Airglow | Physics - Astrophysics of Galaxies
Journal Article
Astrophysical Journal, ISSN 0004-637X, 07/2012, Volume 754, Issue 1, pp. 1 - 8
We present the results of far ultraviolet (FUV) observations of the broad region around the Aquila Rift including the Galactic plane. As compared with various...
ISM: lines and bands | ISM: individual objects (Aquila) | ultraviolet: ISM | MOLECULAR CLOUDS | CS CORE | CO SURVEY | DARK CLOUDS | ORIGINS | EVOLUTION | ASTRONOMY & ASTROPHYSICS | INTERSTELLAR | H-ALPHA | EMISSION | EXTINCTION | Correlation | Dust | Nonuniform | Extinction | Continuums | Emission | Diffusion | Ultraviolet | WAVELENGTHS | CORRELATIONS | PHOTON EMISSION | CARBON MONOXIDE | HYDROGEN | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | ASTRONOMY | FLUORESCENCE | ASTROPHYSICS | STARS | GALAXIES | MILKY WAY | VISIBLE RADIATION | FAR ULTRAVIOLET RADIATION | SCATTERING | COSMIC DUST
ISM: lines and bands | ISM: individual objects (Aquila) | ultraviolet: ISM | MOLECULAR CLOUDS | CS CORE | CO SURVEY | DARK CLOUDS | ORIGINS | EVOLUTION | ASTRONOMY & ASTROPHYSICS | INTERSTELLAR | H-ALPHA | EMISSION | EXTINCTION | Correlation | Dust | Nonuniform | Extinction | Continuums | Emission | Diffusion | Ultraviolet | WAVELENGTHS | CORRELATIONS | PHOTON EMISSION | CARBON MONOXIDE | HYDROGEN | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | ASTRONOMY | FLUORESCENCE | ASTROPHYSICS | STARS | GALAXIES | MILKY WAY | VISIBLE RADIATION | FAR ULTRAVIOLET RADIATION | SCATTERING | COSMIC DUST
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2003, Volume 405, Issue 2, pp. 585 - 590
The distance dependence of interstellar extinction in the direction of the Aquila Rift is investigated using 473 stars observed in the Vilnius photometric...
ISM: clouds | ISM: dust, extinction | ISM: individual objects: Serpens molecular cloud | Stars: fundamental parameters | ISM: individual objects: Aquila Rift | CATALOG | MOLECULAR CLOUDS | ASTRONOMY & ASTROPHYSICS | CLASSIFICATION | STARS | ULTRAVIOLET EXTINCTION | VARIABLES | MILKY-WAY | CO SURVEY | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies
ISM: clouds | ISM: dust, extinction | ISM: individual objects: Serpens molecular cloud | Stars: fundamental parameters | ISM: individual objects: Aquila Rift | CATALOG | MOLECULAR CLOUDS | ASTRONOMY & ASTROPHYSICS | CLASSIFICATION | STARS | ULTRAVIOLET EXTINCTION | VARIABLES | MILKY-WAY | CO SURVEY | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 07/2010, Volume 518, Issue 2, p. L106
The origin and possible universality of the stellar initial mass function (IMF) is a major issue in astrophysics. One of the main objectives of the Herschel...
ISM: individual objects: Aquila rift complex - stars: formation | Stars: formation | ISM: individual objects: Aquila rift complex | stars: formation | ORIGIN | MOLECULAR CLOUDS | ASTRONOMY & ASTROPHYSICS | STAR-FORMATION | INITIAL MASS FUNCTION | MAIN CLOUD | EMISSION | Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics | Physics
ISM: individual objects: Aquila rift complex - stars: formation | Stars: formation | ISM: individual objects: Aquila rift complex | stars: formation | ORIGIN | MOLECULAR CLOUDS | ASTRONOMY & ASTROPHYSICS | STAR-FORMATION | INITIAL MASS FUNCTION | MAIN CLOUD | EMISSION | Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics | Physics
Journal Article
Chinese Astronomy and Astrophysics, ISSN 0275-1062, 2010, Volume 34, Issue 4, pp. 374 - 385
Using the 2m telescope of the Turingia State Observatory at Tauten-berg (TLS), imaging observations in 3 wavebands (H , R and I) are performed in the 16 fields...
ISM—individual: Aquila Rift—stars: emission-line | ISM-individual: Aquila Rift-stars: emission-line | Astronomy | Point sources | Rest | Infrared | Stars | Emission | Latitude | Spectra
ISM—individual: Aquila Rift—stars: emission-line | ISM-individual: Aquila Rift-stars: emission-line | Astronomy | Point sources | Rest | Infrared | Stars | Emission | Latitude | Spectra
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 12/2015, Volume 584, p. A&A 2015
We present and discuss the results of the Herschel Gould Belt survey (HGBS) observations in an similar to 11 deg(2) area of the Aquila molecular cloud complex...
ISM: clouds | Submillimeter: ISM | ISM: individual objects: Aquila Rift complex | Stars: formation | ISM: structure | FORMATION RATES | INITIAL CONDITIONS | MOLECULAR CLOUD | FILAMENTARY STRUCTURES | STAR-FORMATION RATE | LARGE-SCALE | PRESTELLAR CORES | stars: formation | DUST TEMPERATURE | SPITZER C2D | submillimeter: ISM | ASTRONOMY & ASTROPHYSICS | MASS FUNCTION | Algorithms | Clouds | Samples | Spires | Belts | Statistical methods | Photometry | Protostars | Physics - Astrophysics of Galaxies | Galactic Astrophysics | Sciences of the Universe | Astrophysics
ISM: clouds | Submillimeter: ISM | ISM: individual objects: Aquila Rift complex | Stars: formation | ISM: structure | FORMATION RATES | INITIAL CONDITIONS | MOLECULAR CLOUD | FILAMENTARY STRUCTURES | STAR-FORMATION RATE | LARGE-SCALE | PRESTELLAR CORES | stars: formation | DUST TEMPERATURE | SPITZER C2D | submillimeter: ISM | ASTRONOMY & ASTROPHYSICS | MASS FUNCTION | Algorithms | Clouds | Samples | Spires | Belts | Statistical methods | Photometry | Protostars | Physics - Astrophysics of Galaxies | Galactic Astrophysics | Sciences of the Universe | Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 08/2016, Volume 460, Issue 4, pp. 4150 - 4175
We present SCUBA-2 450 mu m and 850 mu m observations of the W40 complex in the Serpens-Aquila region as part of the James Clerk Maxwell Telescope (JCMT) Gould...
Catalogues | Radiative transfer | Submillimetre: general | Stars: formation | HII regions | radiative transfer | AQUILA RIFT | PRESTELLAR CORE POPULATION | YOUNG STELLAR OBJECTS | stars: formation | CLERK-MAXWELL-TELESCOPE | submillimetre: general | H II regions | GIANT MOLECULAR CLOUDS | SURVEY SCUBA-2 OBSERVATIONS | ASTRONOMY & ASTROPHYSICS | SUBMILLIMETER CONTINUUM | MAIN-SEQUENCE STAR | RADIO-SOURCES | catalogues | STAR-FORMING REGION
Catalogues | Radiative transfer | Submillimetre: general | Stars: formation | HII regions | radiative transfer | AQUILA RIFT | PRESTELLAR CORE POPULATION | YOUNG STELLAR OBJECTS | stars: formation | CLERK-MAXWELL-TELESCOPE | submillimetre: general | H II regions | GIANT MOLECULAR CLOUDS | SURVEY SCUBA-2 OBSERVATIONS | ASTRONOMY & ASTROPHYSICS | SUBMILLIMETER CONTINUUM | MAIN-SEQUENCE STAR | RADIO-SOURCES | catalogues | STAR-FORMING REGION
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 466, Issue 3, pp. 2529 - 2541
Filaments in Herschel molecular cloud images are found to exhibit a 'characteristic width'. This finding is in tension with spatial power spectra of the data,...
ISM: individual objects: IC 5146 | ISM: clouds | Methods: statistical | Stars: formation | ISM: individual objects: Aquila Rift | ISM: individual objects: Polaris Flare | LAW | STAR-FORMATION | HERSCHEL | FRAGMENTATION | DISTRIBUTIONS | stars: formation | methods: statistical | ORIGIN | ASTRONOMY & ASTROPHYSICS | DENSE CORES | TURBULENCE | ISM: individual objects Polaris Flare
ISM: individual objects: IC 5146 | ISM: clouds | Methods: statistical | Stars: formation | ISM: individual objects: Aquila Rift | ISM: individual objects: Polaris Flare | LAW | STAR-FORMATION | HERSCHEL | FRAGMENTATION | DISTRIBUTIONS | stars: formation | methods: statistical | ORIGIN | ASTRONOMY & ASTROPHYSICS | DENSE CORES | TURBULENCE | ISM: individual objects Polaris Flare
Journal Article
ASTROPHYSICAL JOURNAL (ISSN 0004-637X), ISSN 0004-637X, 2017, Volume 834, Issue 2, p. 143
We report on new distances and proper motions to seven stars across the Serpens/Aquila complex. The observations were obtained as part of the Gould's Belt...
astrometry | techniques: interferometric | radiation mechanisms: non-thermal-radio continuum: stars | radiation mechanisms: non-thermal | SPITZER C2D SURVEY | EMBEDDED-CLUSTER | AQUILA RIFT | CLOUD CORE | YOUNG STELLAR OBJECTS | INTERSTELLAR CLOUDS | DARK CLOUD | CHANDRA OBSERVATION | radio continuum: stars | ASTRONOMY & ASTROPHYSICS | RADIO-SOURCES | STAR-FORMING REGION
astrometry | techniques: interferometric | radiation mechanisms: non-thermal-radio continuum: stars | radiation mechanisms: non-thermal | SPITZER C2D SURVEY | EMBEDDED-CLUSTER | AQUILA RIFT | CLOUD CORE | YOUNG STELLAR OBJECTS | INTERSTELLAR CLOUDS | DARK CLOUD | CHANDRA OBSERVATION | radio continuum: stars | ASTRONOMY & ASTROPHYSICS | RADIO-SOURCES | STAR-FORMING REGION
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 12/2018, Volume 869, Issue 2, p. L33
We present Gaia-DR2 astrometry of a sample of YSO candidates in Ophiuchus, Serpens Main, and Serpens South/W40 in the Aquila Rift, which had been mainly...
radio continuum: stars | ISM: individual objects (Aquila Rift complex, Ophiuchus) | astrometry | techniques: interferometric | radiation mechanisms: nonthermal | ASTRONOMY & ASTROPHYSICS | STAR-FORMING REGIONS
radio continuum: stars | ISM: individual objects (Aquila Rift complex, Ophiuchus) | astrometry | techniques: interferometric | radiation mechanisms: nonthermal | ASTRONOMY & ASTROPHYSICS | STAR-FORMING REGIONS
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2012, Volume 542, p. A81
We present a multi-scale, multi-wavelength source extraction algorithm called getsources. Although it has been designed primarily for use in the far-infrared...
Techniques: photometric | Infrared: ISM | Techniques: image processing | Submillimeter: ISM | Methods: data analysis | Stars: formation | methods: data analysis | techniques: photometric | INITIAL HIGHLIGHTS | AQUILA RIFT | STAR-FORMATION | infrared: ISM | HERSCHEL | stars: formation | PROTOCLUSTERS | ROSETTE MOLECULAR CLOUD | CATALOG | techniques: image processing | submillimeter: ISM | ASTRONOMY & ASTROPHYSICS | DENSE CORES | PROTOSTARS | TURBULENCE
Techniques: photometric | Infrared: ISM | Techniques: image processing | Submillimeter: ISM | Methods: data analysis | Stars: formation | methods: data analysis | techniques: photometric | INITIAL HIGHLIGHTS | AQUILA RIFT | STAR-FORMATION | infrared: ISM | HERSCHEL | stars: formation | PROTOCLUSTERS | ROSETTE MOLECULAR CLOUD | CATALOG | techniques: image processing | submillimeter: ISM | ASTRONOMY & ASTROPHYSICS | DENSE CORES | PROTOSTARS | TURBULENCE
Journal Article
Astrophysical Journal, ISSN 0004-637X, 06/2015, Volume 806, Issue 2, pp. 1 - 13
We present an HCO+ J = 3. 2 survey of Class 0+I and Flat SED young stellar objects (YSOs) found in the Gould Belt clouds by surveys with Spitzer. Our goal is...
ISM: clouds | dust, extinction | galaxies: ISM | infrared: stars | galaxies: star formation | SPITZER C2D SURVEY | MOLECULAR CLOUD | galaxies: star formation Supporting material: machine-readable table | AQUILA RIFT | PLANET FORMATION | DISK EVOLUTION | YOUNG STELLAR OBJECTS | INTERSTELLAR CLOUDS | CORONA AUSTRALIS | MASS STAR-FORMATION | NEARBY DENSE CORES | ASTRONOMY & ASTROPHYSICS | Clouds | Star formation | Galaxies | Extinction | Flats | Belts | Criteria | Protostars
ISM: clouds | dust, extinction | galaxies: ISM | infrared: stars | galaxies: star formation | SPITZER C2D SURVEY | MOLECULAR CLOUD | galaxies: star formation Supporting material: machine-readable table | AQUILA RIFT | PLANET FORMATION | DISK EVOLUTION | YOUNG STELLAR OBJECTS | INTERSTELLAR CLOUDS | CORONA AUSTRALIS | MASS STAR-FORMATION | NEARBY DENSE CORES | ASTRONOMY & ASTROPHYSICS | Clouds | Star formation | Galaxies | Extinction | Flats | Belts | Criteria | Protostars
Journal Article
Astrophysical Journal, ISSN 0004-637X, 12/2016, Volume 833, Issue 2, p. 204
Filamentary structures are ubiquitous in molecular clouds, and have been recently argued to play an important role in regulating the size and mass of embedded...
ISM: clouds | molecular data | radio lines: ISM | line: profiles | galaxies: star formation | ISM: kinematics and dynamics | MOLECULAR CLOUDS | AQUILA RIFT | STAR-FORMATION | CLUSTER FORMATION | GOULD BELT SURVEY | FREE-FALL TIME | CLUMP DISTRIBUTION | ASTRONOMY & ASTROPHYSICS | DENSE CORES | INFRARED DARK CLOUD | TURBULENT CONVERGING FLOWS | Physics - Astrophysics of Galaxies
ISM: clouds | molecular data | radio lines: ISM | line: profiles | galaxies: star formation | ISM: kinematics and dynamics | MOLECULAR CLOUDS | AQUILA RIFT | STAR-FORMATION | CLUSTER FORMATION | GOULD BELT SURVEY | FREE-FALL TIME | CLUMP DISTRIBUTION | ASTRONOMY & ASTROPHYSICS | DENSE CORES | INFRARED DARK CLOUD | TURBULENT CONVERGING FLOWS | Physics - Astrophysics of Galaxies
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 06/2011, Volume 734, Issue 1, p. 63
The Serpens South embedded cluster, which is located in the constricted part of a long, filamentary, infrared dark cloud, is believed to be in a very early...
stars: formation | open clusters and associations: individual (Serpens South) | polarization | infrared: stars | ISM: structure | ISM: magnetic fields | CORES | AQUILA RIFT | CAMERA | DRIVEN | CLUSTER FORMATION | INTERSTELLAR CLOUDS | DARK CLOUDS | GOULD BELT SURVEY | OUTFLOWS | ASTRONOMY & ASTROPHYSICS | TURBULENCE | Physics - Solar and Stellar Astrophysics | MAGNETIC FIELDS | NEAR INFRARED RADIATION | FILAMENTS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | POLARIMETRY | CLOUDS | ELECTROMAGNETIC RADIATION | INFRARED RADIATION | RADIATIONS | POLARIZATION
stars: formation | open clusters and associations: individual (Serpens South) | polarization | infrared: stars | ISM: structure | ISM: magnetic fields | CORES | AQUILA RIFT | CAMERA | DRIVEN | CLUSTER FORMATION | INTERSTELLAR CLOUDS | DARK CLOUDS | GOULD BELT SURVEY | OUTFLOWS | ASTRONOMY & ASTROPHYSICS | TURBULENCE | Physics - Solar and Stellar Astrophysics | MAGNETIC FIELDS | NEAR INFRARED RADIATION | FILAMENTS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | POLARIMETRY | CLOUDS | ELECTROMAGNETIC RADIATION | INFRARED RADIATION | RADIATIONS | POLARIZATION
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 06/2014, Volume 787, Issue 2, pp. L18 - 6
We use PACS and SPIRE continuum data at 160 mu m, 250 mu m, 350 mu m, and 500 mu m from the Herschel Gould Belt Survey to sample seven clumps in Perseus: B1,...
stars: formation | dust, extinction | ISM: individual objects (Perseus) | stars: protostars | AQUILA RIFT | HERSCHEL | INTERSTELLAR CLOUDS | EXTRACTION | EVOLUTION | FILAMENTS | STAR-FORMATION RATES | TEMPERATURE | ASTRONOMY & ASTROPHYSICS | ORION | DUST PROPERTIES | Correlation | Star formation | Clumps | Density distribution | Density | Photometry | Columns (structural) | Protostars | Physics - Solar and Stellar Astrophysics | DENSITY | STAR CLUSTERS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | STAR EVOLUTION | CLOUDS | PROTOSTARS | STARS | DETECTION | EFFICIENCY | FEEDBACK | COSMIC DUST
stars: formation | dust, extinction | ISM: individual objects (Perseus) | stars: protostars | AQUILA RIFT | HERSCHEL | INTERSTELLAR CLOUDS | EXTRACTION | EVOLUTION | FILAMENTS | STAR-FORMATION RATES | TEMPERATURE | ASTRONOMY & ASTROPHYSICS | ORION | DUST PROPERTIES | Correlation | Star formation | Clumps | Density distribution | Density | Photometry | Columns (structural) | Protostars | Physics - Solar and Stellar Astrophysics | DENSITY | STAR CLUSTERS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | STAR EVOLUTION | CLOUDS | PROTOSTARS | STARS | DETECTION | EFFICIENCY | FEEDBACK | COSMIC DUST
Journal Article
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Full Text
Abundant cyanopolyynes as a probe of infall in the Serpens South cluster-forming region
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 12/2013, Volume 436, Issue 2, pp. 1513 - 1529
We have detected bright HC7N J = 21 − 20 emission towards multiple locations in the Serpens South cluster-forming region using the K-Band Focal Plane Array at...
radio lines:ISM | Astrochemistry | ISM:abundances | Stars:formation | AMMONIA | DARK CLOUD CORES | STARLESS CORES | AQUILA RIFT | ISM: abundances | INTERSTELLAR CLOUDS | stars: formation | CARBON-CHAIN MOLECULES | GOULD BELT SURVEY | radio lines: ISM | ASTRONOMY & ASTROPHYSICS | DENSE CORES | CHEMISTRY | astrochemistry | MOLECULAR LINE OBSERVATIONS | Physics - Astrophysics of Galaxies
radio lines:ISM | Astrochemistry | ISM:abundances | Stars:formation | AMMONIA | DARK CLOUD CORES | STARLESS CORES | AQUILA RIFT | ISM: abundances | INTERSTELLAR CLOUDS | stars: formation | CARBON-CHAIN MOLECULES | GOULD BELT SURVEY | radio lines: ISM | ASTRONOMY & ASTROPHYSICS | DENSE CORES | CHEMISTRY | astrochemistry | MOLECULAR LINE OBSERVATIONS | Physics - Astrophysics of Galaxies
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 08/2014, Volume 790, Issue 2, pp. L19 - 6
We present the N2H+ (J = 1 -> 0) map of the Serpens South molecular cloud obtained as part of the CARMA Large Area Star Formation Survey. The observations...
ISM: individual objects (Serpens South) | stars: formation | ISM: clouds | ISM: structure | ISM: kinematics and dynamics | EXCITATION | AQUILA RIFT | PRESTELLAR CORES | REGION | GOULD BELT SURVEY | ASTRONOMY & ASTROPHYSICS | INFRARED DARK CLOUD | FLOWS | CLUSTER | Turbulence | Dust | Star formation | Molecular clouds | Filaments | Continuums | Emission | Evolution | PLASMA FILAMENT | VELOCITY | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | STAR EVOLUTION | CLOUDS | RESOLUTION | STARS | TURBULENCE | SPATIAL DISTRIBUTION | COSMIC DUST
ISM: individual objects (Serpens South) | stars: formation | ISM: clouds | ISM: structure | ISM: kinematics and dynamics | EXCITATION | AQUILA RIFT | PRESTELLAR CORES | REGION | GOULD BELT SURVEY | ASTRONOMY & ASTROPHYSICS | INFRARED DARK CLOUD | FLOWS | CLUSTER | Turbulence | Dust | Star formation | Molecular clouds | Filaments | Continuums | Emission | Evolution | PLASMA FILAMENT | VELOCITY | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | STAR EVOLUTION | CLOUDS | RESOLUTION | STARS | TURBULENCE | SPATIAL DISTRIBUTION | COSMIC DUST
Journal Article