Astrophysical Journal, ISSN 0004-637X, 01/2015, Volume 798, Issue 1, pp. 31 - 14
NGC 1266 is a nearby lenticular galaxy that harbors a massive outflow of molecular gas powered by the mechanical energy of an active galactic nucleus (AGN). It...
Galaxies: nuclei | Galaxies: elliptical and lenticular, cD | Galaxies: evolution | Radio continuum: galaxies | Galaxies: ISM | Galaxies: star formation | Galaxies: individual (NGC 1266) | Molecular data | Submillimeter: galaxies | NEARBY GALAXIES | ATLAS(3D) PROJECT | galaxies: evolution | galaxies: star formation | DRIVEN MOLECULAR OUTFLOW | STEPHANS QUINTET | galaxies: elliptical and lenticular, cD | RADIO GALAXIES | galaxies: individual (NGC 1266) | submillimeter: galaxies | EARLY-TYPE GALAXIES | molecular data | ACTIVE GALACTIC NUCLEI | SPECTRAL ENERGY-DISTRIBUTIONS | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | SPITZER-SPACE-TELESCOPE | galaxies: nuclei | radio continuum: galaxies | ULTRALUMINOUS INFRARED GALAXIES | Active galactic nuclei | Turbulence | Wavelengths | Star formation | Fluid dynamics | Galaxy formation | Feedback | Jets | Outflow | GRAVITATIONAL COLLAPSE | PHOTON EMISSION | BLACK HOLES | DENSITY | STAR CLUSTERS | QUASARS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | JETS | STARS | FEEDBACK | GALAXY NUCLEI | FAR INFRARED RADIATION
Galaxies: nuclei | Galaxies: elliptical and lenticular, cD | Galaxies: evolution | Radio continuum: galaxies | Galaxies: ISM | Galaxies: star formation | Galaxies: individual (NGC 1266) | Molecular data | Submillimeter: galaxies | NEARBY GALAXIES | ATLAS(3D) PROJECT | galaxies: evolution | galaxies: star formation | DRIVEN MOLECULAR OUTFLOW | STEPHANS QUINTET | galaxies: elliptical and lenticular, cD | RADIO GALAXIES | galaxies: individual (NGC 1266) | submillimeter: galaxies | EARLY-TYPE GALAXIES | molecular data | ACTIVE GALACTIC NUCLEI | SPECTRAL ENERGY-DISTRIBUTIONS | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | SPITZER-SPACE-TELESCOPE | galaxies: nuclei | radio continuum: galaxies | ULTRALUMINOUS INFRARED GALAXIES | Active galactic nuclei | Turbulence | Wavelengths | Star formation | Fluid dynamics | Galaxy formation | Feedback | Jets | Outflow | GRAVITATIONAL COLLAPSE | PHOTON EMISSION | BLACK HOLES | DENSITY | STAR CLUSTERS | QUASARS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | JETS | STARS | FEEDBACK | GALAXY NUCLEI | FAR INFRARED RADIATION
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 04/2012, Volume 749, Issue 1
We describe cosmological galaxy formation simulations with the adaptive mesh refinement code Enzo that incorporate a star formation prescription regulated by...
LYMAN-BREAK GALAXIES | EARLY RELEASE SCIENCE | COLD DARK-MATTER | ULTRA-DEEP-FIELD | COSMIC STRUCTURE FORMATION | methods: numerical | HIGH-REDSHIFT GALAXIES | galaxies: halos | cosmology: theory | galaxies: dwarf | galaxies: formation | SIMILAR-TO 7 | GIANT MOLECULAR CLOUDS | ASTRONOMY & ASTROPHYSICS | KENNICUTT-SCHMIDT RELATION | PIECEWISE PARABOLIC METHOD
LYMAN-BREAK GALAXIES | EARLY RELEASE SCIENCE | COLD DARK-MATTER | ULTRA-DEEP-FIELD | COSMIC STRUCTURE FORMATION | methods: numerical | HIGH-REDSHIFT GALAXIES | galaxies: halos | cosmology: theory | galaxies: dwarf | galaxies: formation | SIMILAR-TO 7 | GIANT MOLECULAR CLOUDS | ASTRONOMY & ASTROPHYSICS | KENNICUTT-SCHMIDT RELATION | PIECEWISE PARABOLIC METHOD
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 12/2015, Volume 584, p. A67
Context. Filamentary structures in the interstellar medium are crucial ingredients of the star formation process. They fragment to form individual star-forming...
Stars: individual: IRDC 18223 | ISM: clouds | Stars: early-type | Stars: formation | ISM: structure | Stars: massive | MOLECULAR CLOUDS | DENSITY STRUCTURE | HERSCHEL | G11.11-0.12 | stars: formation | stars: early-type | HELICAL FIELDS | DUST | stars: individual: IRDC 18223 | CORE FORMATION | ASTRONOMY & ASTROPHYSICS | stars: massive | INFRARED-DARK CLOUD | PROTOSTELLAR CANDIDATES | GRAVITATIONAL INFALL | Clouds | Star formation | Filaments | Continuums | Formations | Interferometers | Cylinders | Fragmentation
Stars: individual: IRDC 18223 | ISM: clouds | Stars: early-type | Stars: formation | ISM: structure | Stars: massive | MOLECULAR CLOUDS | DENSITY STRUCTURE | HERSCHEL | G11.11-0.12 | stars: formation | stars: early-type | HELICAL FIELDS | DUST | stars: individual: IRDC 18223 | CORE FORMATION | ASTRONOMY & ASTROPHYSICS | stars: massive | INFRARED-DARK CLOUD | PROTOSTELLAR CANDIDATES | GRAVITATIONAL INFALL | Clouds | Star formation | Filaments | Continuums | Formations | Interferometers | Cylinders | Fragmentation
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2013, Volume 428, Issue 4, pp. 3121 - 3138
We present a new statistical method to determine the relationship between the stellar masses of galaxies and the masses of their host dark matter haloes over...
Theory - dark matter | High-redshift - galaxies | Stellar content - cosmology | Evolution - galaxies | Galaxies | Statistics - galaxies | FORMATION RATES | EARLY RELEASE SCIENCE | ELLIPTIC GALAXIES | galaxies: evolution | PROBE WMAP OBSERVATIONS | GOODS-S FIELD | LUMINOSITY FUNCTION | galaxies: high-redshift | COSMOLOGICAL SIMULATIONS | cosmology: theory | galaxies: statistics | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | SPITZER-SPACE-TELESCOPE | STELLAR MASS FUNCTION | galaxies: stellar content | dark matter | Physics - Cosmology and Nongalactic Astrophysics
Theory - dark matter | High-redshift - galaxies | Stellar content - cosmology | Evolution - galaxies | Galaxies | Statistics - galaxies | FORMATION RATES | EARLY RELEASE SCIENCE | ELLIPTIC GALAXIES | galaxies: evolution | PROBE WMAP OBSERVATIONS | GOODS-S FIELD | LUMINOSITY FUNCTION | galaxies: high-redshift | COSMOLOGICAL SIMULATIONS | cosmology: theory | galaxies: statistics | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | SPITZER-SPACE-TELESCOPE | STELLAR MASS FUNCTION | galaxies: stellar content | dark matter | Physics - Cosmology and Nongalactic Astrophysics
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 08/2017, Volume 469, Issue 2, pp. 2263 - 2285
The inner few hundred parsecs of the Milky Way harbours gas densities, pressures, velocity dispersions, an interstellar radiation field and a cosmic ray...
FORMATION RATE INDICATORS | SGR A-ASTERISK | SAGITTARIUS B2 | CENTRAL MOLECULAR ZONE | YOUNG STELLAR OBJECTS | stars: formation | H II regions | EARLY-TYPE GALAXIES | Galaxy: centre | CENTER CLOUD G0.253+0.016 | ASTRONOMY & ASTROPHYSICS | ISM: clouds | INITIAL MASS FUNCTION | RECOMBINATION LINE OBSERVATIONS | MILKY-WAY | Physics - Astrophysics of Galaxies
FORMATION RATE INDICATORS | SGR A-ASTERISK | SAGITTARIUS B2 | CENTRAL MOLECULAR ZONE | YOUNG STELLAR OBJECTS | stars: formation | H II regions | EARLY-TYPE GALAXIES | Galaxy: centre | CENTER CLOUD G0.253+0.016 | ASTRONOMY & ASTROPHYSICS | ISM: clouds | INITIAL MASS FUNCTION | RECOMBINATION LINE OBSERVATIONS | MILKY-WAY | Physics - Astrophysics of Galaxies
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2014, Volume 437, Issue 2, pp. 1791 - 1807
We have used the well-selected sample of ∼1750 embedded, young, massive stars identified by the Red MSX Source (RMS) survey to investigate the Galactic...
Molecules -galaxy | Formation - ISM | Structure | Kinematics and dynamics - galaxy | Stars | Early-type - stars | Galaxy: structure | Galaxy: kinematics and dynamics | OUTER GALAXY | (CO)-C-13 OBSERVATIONS | H-II REGIONS | GIANT MOLECULAR CLOUD | SOLAR CIRCLE | stars: formation | KINEMATIC DISTANCE AMBIGUITY | stars: early-type | MSX SOURCE SURVEY | SPIRAL STRUCTURE | ISM: molecules | ASTRONOMY & ASTROPHYSICS | MILKY-WAY | HII-REGIONS | Physics - Astrophysics of Galaxies
Molecules -galaxy | Formation - ISM | Structure | Kinematics and dynamics - galaxy | Stars | Early-type - stars | Galaxy: structure | Galaxy: kinematics and dynamics | OUTER GALAXY | (CO)-C-13 OBSERVATIONS | H-II REGIONS | GIANT MOLECULAR CLOUD | SOLAR CIRCLE | stars: formation | KINEMATIC DISTANCE AMBIGUITY | stars: early-type | MSX SOURCE SURVEY | SPIRAL STRUCTURE | ISM: molecules | ASTRONOMY & ASTROPHYSICS | MILKY-WAY | HII-REGIONS | Physics - Astrophysics of Galaxies
Journal Article
Reports on Progress in Physics, ISSN 0034-4885, 10/2003, Volume 66, Issue 10, pp. 1651 - 1697
Our current understanding of the physical processes of star formation is reviewed, with emphasis on processes occurring in molecular clouds like those observed...
ANGULAR-MOMENTUM TRANSPORT | PHYSICS, MULTIDISCIPLINARY | CLOSE BINARY-SYSTEMS | SELF-SIMILAR COLLAPSE | T-TAURI DISKS | MOLECULAR CLOUD CORES | EARLY STELLAR EVOLUTION | ROTATING ISOTHERMAL CLOUDS | INITIAL MASS FUNCTION | PRE-MAIN-SEQUENCE | SOLAR-TYPE STARS | 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
ANGULAR-MOMENTUM TRANSPORT | PHYSICS, MULTIDISCIPLINARY | CLOSE BINARY-SYSTEMS | SELF-SIMILAR COLLAPSE | T-TAURI DISKS | MOLECULAR CLOUD CORES | EARLY STELLAR EVOLUTION | ROTATING ISOTHERMAL CLOUDS | INITIAL MASS FUNCTION | PRE-MAIN-SEQUENCE | SOLAR-TYPE STARS | 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
Astrophysical Journal, ISSN 0004-637X, 06/2013, Volume 770, Issue 1, pp. 1 - 36
We present a robust method to constrain average galaxy star formation rates (SFRs), star formation histories (SFHs), and the intracluster light (ICL) as a...
methods: numerical | galaxies: evolution | dark matter galaxies: abundances | LYMAN-BREAK GALAXIES | OBSERVATIONS COSMOLOGICAL INTERPRETATION | EARLY RELEASE SCIENCE | UV LUMINOSITY FUNCTION | MEDIUM-BAND SURVEY | K-SELECTED GALAXIES | FORMATION RATE DENSITY | EXTRAGALACTIC LEGACY SURVEY | BRIGHTEST CLUSTER GALAXIES | ASTRONOMY & ASTROPHYSICS | STELLAR MASS FUNCTION | galaxies: abundances | dark matter | Galactic halos | Uncertainty | Halos | Star formation | Dark matter | Galaxies | Stellar mass | Star formation rate | Physics - Cosmology and Nongalactic Astrophysics | DENSITY | CALIBRATION | RED SHIFT | NONLUMINOUS MATTER | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | BUILDUP | MASS | STARS | GALACTIC EVOLUTION | GALAXIES | BARYONS
methods: numerical | galaxies: evolution | dark matter galaxies: abundances | LYMAN-BREAK GALAXIES | OBSERVATIONS COSMOLOGICAL INTERPRETATION | EARLY RELEASE SCIENCE | UV LUMINOSITY FUNCTION | MEDIUM-BAND SURVEY | K-SELECTED GALAXIES | FORMATION RATE DENSITY | EXTRAGALACTIC LEGACY SURVEY | BRIGHTEST CLUSTER GALAXIES | ASTRONOMY & ASTROPHYSICS | STELLAR MASS FUNCTION | galaxies: abundances | dark matter | Galactic halos | Uncertainty | Halos | Star formation | Dark matter | Galaxies | Stellar mass | Star formation rate | Physics - Cosmology and Nongalactic Astrophysics | DENSITY | CALIBRATION | RED SHIFT | NONLUMINOUS MATTER | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | BUILDUP | MASS | STARS | GALACTIC EVOLUTION | GALAXIES | BARYONS
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2012, Volume 426, Issue 4, pp. 3008 - 3040
Abstract We present a theoretical framework in which bound stellar clusters arise naturally at the high-density end of the hierarchy of the interstellar medium...
stars: formation | galaxies: starburst | galaxies: star clusters: general | galaxies: ISM | galaxies: stellar content | Galaxies: stellar content | Galaxies: star clusters: general | Stars: formation | Galaxies: starburst | Galaxies: ISM | COLD DARK-MATTER | DYNAMICAL EVOLUTION | SIMILAR-TO 2 | BLUE COMPACT GALAXIES | INTERSTELLAR-MEDIUM | EARLY-TYPE GALAXIES | GIANT MOLECULAR CLOUDS | ALPHA VELOCITY-FIELDS | ASTRONOMY & ASTROPHYSICS | INITIAL MASS FUNCTION | GLOBULAR-CLUSTERS | Analysis | Astronomy | Doppler effect | Star & galaxy formation | Spectrum analysis
stars: formation | galaxies: starburst | galaxies: star clusters: general | galaxies: ISM | galaxies: stellar content | Galaxies: stellar content | Galaxies: star clusters: general | Stars: formation | Galaxies: starburst | Galaxies: ISM | COLD DARK-MATTER | DYNAMICAL EVOLUTION | SIMILAR-TO 2 | BLUE COMPACT GALAXIES | INTERSTELLAR-MEDIUM | EARLY-TYPE GALAXIES | GIANT MOLECULAR CLOUDS | ALPHA VELOCITY-FIELDS | ASTRONOMY & ASTROPHYSICS | INITIAL MASS FUNCTION | GLOBULAR-CLUSTERS | Analysis | Astronomy | Doppler effect | Star & galaxy formation | Spectrum analysis
Journal Article
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Variations in the Galactic star formation rate and density thresholds for star formation
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2013, Volume 429, Issue 2, pp. 987 - 1000
The conversion of gas into stars is a fundamental process in astrophysics and cosmology. Stars are known to form from the gravitational collapse of dense...
Clouds - ISM | Evolution - Galaxy | Formation - stars | Centre | Masers - stars | Massive - ISM | NEARBY GALAXIES | GHZ METHANOL MASERS | ISM: evolution | PLANE SURVEY | FORMING REGIONS | masers | CENTRAL MOLECULAR ZONE | YOUNG STELLAR OBJECTS | stars: formation | EARLY-TYPE GALAXIES | Galaxy: centre | ASTRONOMY & ASTROPHYSICS | stars: massive | ISM: clouds | CIRCUMSTELLAR DISKS | INITIAL MASS FUNCTION | MILKY-WAY
Clouds - ISM | Evolution - Galaxy | Formation - stars | Centre | Masers - stars | Massive - ISM | NEARBY GALAXIES | GHZ METHANOL MASERS | ISM: evolution | PLANE SURVEY | FORMING REGIONS | masers | CENTRAL MOLECULAR ZONE | YOUNG STELLAR OBJECTS | stars: formation | EARLY-TYPE GALAXIES | Galaxy: centre | ASTRONOMY & ASTROPHYSICS | stars: massive | ISM: clouds | CIRCUMSTELLAR DISKS | INITIAL MASS FUNCTION | MILKY-WAY
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2014, Volume 563, pp. A97 - np
Understanding the chemical evolution of young (high-mass) star-forming regions is a central topic in star formation research. Chemistry is employed as a unique...
Evolution | ISM: molecules | Stars: early-type | Stars: formation | DUST CONTINUUM | PHYSICAL-PROPERTIES | PROTOPLANETARY DISKS | INFRARED-DARK CLOUDS | INTERSTELLAR-MEDIUM | FORMING REGIONS | evolution
Evolution | ISM: molecules | Stars: early-type | Stars: formation | DUST CONTINUUM | PHYSICAL-PROPERTIES | PROTOPLANETARY DISKS | INFRARED-DARK CLOUDS | INTERSTELLAR-MEDIUM | FORMING REGIONS | evolution