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Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2019, Volume 484, Issue 4, pp. 5734 - 5754
The evolution of molecular clouds in galactic centres is thought to differ from that in galactic discs due to a significant influence of the external... 
Galaxy: Centre | ISM: Evolution | ISM: Kinematics and dynamics | Stars: Formation | ISM: Clouds | Galaxies: ISM | ROTATION | ISM: evolution | STARBURSTS | ISM: kinematics and dynamics | ENVIRONMENT | STAR-FORMATION | COLLISION | stars: formation | PLANE SURVEY HOPS | Galaxy: centre | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | GAS | ISM: clouds | CONTINUUM | GALAXIES | MILKY-WAY
Journal Article
by Keto, E
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 09/2007, Volume 666, Issue 2, pp. 976 - 981
The hypothesis that massive stars form by accretion can be investigated by simple analytical calculations that describe the effect that the formation of a... 
SYSTEM | PROTOSTELLAR DISKS | stars : early-type | H-II REGIONS | MAIN-SEQUENCE | HII regions | RADIATIVE-TRANSFER | IRAS 20126+4104 | EVOLUTION | stars : formation | ASTRONOMY & ASTROPHYSICS | YOUNG STAR | MOLECULAR GAS | ROTATING-DISK
Journal Article
Applied and Environmental Microbiology, ISSN 0099-2240, 03/2005, Volume 71, Issue 3, pp. 1148 - 1154
Amplified fragment length polymorphism (AFLP) analysis was applied to characterize 33 group I and 37 group II Clostridium botulinum strains. Four restriction... 
Journal Article
Applied and Environmental Microbiology, ISSN 0099-2240, 03/2005, Volume 71, Issue 3, p. 1148
  Amplified fragment length polymorphism (AFLP) analysis was applied to characterize 33 group I and 37 group II Clostridium botulinum strains. Four restriction... 
DNA fingerprints | Analysis | Bacteria | Polymorphism
Journal Article
Applied and Environmental Microbiology, ISSN 0099-2240, 03/2005, Volume 71, Issue 3, p. 1148
Journal Article
by Keto, E
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 12/2003, Volume 599, Issue 2, pp. 1196 - 1206
The formation of massive stars may take place at relatively low accretion rates over a long period of time if the accretion can continue past the onset of core... 
PHYSICAL-PROPERTIES | MOLECULAR CLOUDS | accretion, accretion disks | IRAS POINT SOURCES | CONTINUUM OBSERVATIONS | H-II REGIONS | MAIN-SEQUENCE | HII regions | FORMING REGION | stars : formation | STELLAR MODELS | ASTRONOMY & ASTROPHYSICS | VLA OBSERVATIONS | RECOMBINATION LINE OBSERVATIONS
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 07/2017, Volume 603, p. L1
Pre-stellar cores represent the initial conditions in the process of star and planet formation, therefore it is important to study their physical and chemical... 
Methods: observational | Astrochemistry | ISM: clouds | Radiative transfer | ISM: molecules | Line: profiles | Stellar cores | Cold gas | Molecular structure | Volatility | Chemical reactions | Abundance | Rotation | Molecular chains | Cores | Hyperfine structure | Organic chemistry | Ammonia | Initial conditions | Spectral resolution | Planet formation | Spectral sensitivity | Interferometry
Journal Article
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