Physical characterization of southern massive star‐forming regions using Parkes NH3 observations

Physical characterization of southern massive star‐forming regions using Parkes NH3 observations

Source :

• Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2010-03.

Descripteurs français

• Pascal (Inist)
  • Ammoniac, Continuum, Densité colonne, Densité flux, Densité spectrale énergie, Dispersion vitesse, Etoile massive, Etoile premier type, Formation stellaire, Maser, Opacité, Paramètre physique, Principe de complémentarité, Profil raie, Propriété physique, Proto étoile, Région formation stellaire, Transition inversion, Turbulence.
• Wicri :
  • topic : Méthanol.

English descriptors

• KwdEn :
  • Active star formation, Ammonia, Ammonia data, Ammonia observations, Ammonia transitions, Arizona press, Ascension, Australia telescope, Baseline, Baseline variations, Bayesian, Bayesian inference, Bayesian inference method, Beuther, Black line, Blue line, Clump, Column density, Complementarity, Constraint, Continuum, Continuum mass, Continuum observations, Cumulative distribution, Cumulative distribution plot, Cumulative distribution plots, Cumulative distributions, Cumulative fraction, Detection rates, Different classes, Dust emission, Dust temperature, Dust temperatures, Earliest stages, Early type stars, Error bars, Evolutionary status, Excellent agreement, Excellent candidates, Flux density, Form stars, Free parameters, Gain elevation correction, Galactic centre, Good constraints, Individual classes, Individual sources, Inversion transition, Inversion transitions, Irdcs, Journal compilation, Kinetic temperature, Kinetic temperatures, Larger error bars, Line observations, Line shape, Line study, Linewidth, Linewidths, Little distinction, Longmore, Lower limit, Luminosity, Main flux, Maser, Maser sources, Masers, Mass stars, Massive regions, Massive regions table, Massive star, Massive star birth, Massive star formation, Massive stars, Maximum mass, Median, Median value, Menten, Methanol, Methanol maser, Methanol maser associations, Methanol maser radio continuum association, Millimetre, Millimetre continuum, Millimetre continuum sources, Minier, Mmonly sources, Mnras, Modelled, Modelling, Nnh3, Null hypothesis, Online version, Opacity, Optical depth, Optical depths, Other classes, Other half, Parameter, Parameter determinations, Parameter space, Parkes, Parkes ammonia, Parkes telescope, Physical parameter, Physical parameters, Physical properties, Pillai, Probability curve, Probability curves, Probability distributions, Protostars, Protostellar objects, Radio continuum associations, Radio continuum source, Resolution observations, Rest velocity, Right ascension, Right ascension order, Robust, Robust detections, Rotational temperature, Same population, Sample ranges, Schnee sargent, Simba, Simba sample, Simba sources, Small number, Smaller linewidths, Source class, Source declination, Source mass, Source parameters, Source temperature, Spectral energy distribution, Sridharan, Standard deviation, Star formation, Star formation activity, Star formation sample, Starless, Starless cores, Stellar formation region, Thin emission, Total column density, Tting, Turbulence, Upper limit, Upper limits, Velocity components, Velocity dispersion, Virial, Virial mass, Virial parameter, Walmsley, Whilst, Whilst class.
• Teeft :
  • Active star formation, Ammonia, Ammonia data, Ammonia observations, Ammonia transitions, Arizona press, Ascension, Australia telescope, Baseline, Baseline variations, Bayesian, Bayesian inference, Bayesian inference method, Beuther, Black line, Blue line, Clump, Column density, Constraint, Continuum, Continuum mass, Continuum observations, Cumulative distribution, Cumulative distribution plot, Cumulative distribution plots, Cumulative distributions, Cumulative fraction, Detection rates, Different classes, Dust emission, Dust temperature, Dust temperatures, Earliest stages, Error bars, Evolutionary status, Excellent agreement, Excellent candidates, Flux density, Form stars, Free parameters, Gain elevation correction, Galactic centre, Good constraints, Individual classes, Individual sources, Inversion transitions, Irdcs, Journal compilation, Kinetic temperature, Kinetic temperatures, Larger error bars, Line observations, Line study, Linewidth, Linewidths, Little distinction, Longmore, Lower limit, Luminosity, Main flux, Maser, Maser sources, Mass stars, Massive regions, Massive regions table, Massive star, Massive star birth, Massive star formation, Massive stars, Maximum mass, Median, Median value, Menten, Methanol, Methanol maser, Methanol maser associations, Methanol maser radio continuum association, Millimetre, Millimetre continuum, Millimetre continuum sources, Minier, Mmonly sources, Mnras, Modelled, Modelling, Nnh3, Null hypothesis, Online version, Optical depth, Optical depths, Other classes, Other half, Parameter, Parameter determinations, Parameter space, Parkes, Parkes ammonia, Parkes telescope, Physical parameters, Physical properties, Pillai, Probability curve, Probability curves, Probability distributions, Protostars, Protostellar objects, Radio continuum associations, Radio continuum source, Resolution observations, Rest velocity, Right ascension, Right ascension order, Robust, Robust detections, Rotational temperature, Same population, Sample ranges, Schnee sargent, Simba, Simba sample, Simba sources, Small number, Smaller linewidths, Source class, Source declination, Source mass, Source parameters, Source temperature, Sridharan, Standard deviation, Star formation, Star formation activity, Star formation sample, Starless, Starless cores, Thin emission, Total column density, Tting, Upper limit, Upper limits, Velocity components, Virial, Virial mass, Virial parameter, Walmsley, Whilst, Whilst class.

Abstract

• https://api.istex.fr/document/9E9A54280DA8865532DC0DECEC4812D3BCB37DA7/fulltext/pdf

Affiliations:

• Australie, France, Royaume-Uni, États-Unis
• Massachusetts, Île-de-France
• Gif‐sur‐Yvette

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