Search results for "HII region"

showing 2 items of 2 documents

The Gaia-ESO Survey: Dynamics of ionized and neutral gas in the Lagoon nebula (M 8)

2017

Aims. We present a spectroscopic study of the dynamics of the ionized and neutral gas throughout the Lagoon nebula (M 8), using VLT-FLAMES data from the Gaia-ESO Survey. The new data permit exploration of the physical connections between the nebular gas and the stellar population of the associated star cluster NGC 6530. Methods. We characterized through spectral fitting emission lines of Hα, [N II] and [S II] doublets, [O III], and absorption lines of sodium D doublet, using data from the FLAMES-Giraffe and UVES spectrographs, on more than 1000 sightlines toward the entire face of the Lagoon nebula. Gas temperatures are derived from line-width comparisons, densities from the [S II] doublet …

HII regionsStellar populationAstrophysics::High Energy Astrophysical PhenomenaDoubly ionized oxygenFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences7. Clean energy0103 physical sciencesProtostarAstrophysics::Solar and Stellar AstrophysicsHII region010303 astronomy & astrophysicsISM: individual objects: Lagoon nebulaSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsO-type starISM: generalPhysicsNebulageneral [ISM]010308 nuclear & particles physicsMolecular cloudHII regions; ISM: general; ISM: individual objects: Lagoon nebula; Astronomy and Astrophysics; Space and Planetary ScienceAstronomy and AstrophysicsAstrophysics - Astrophysics of Galaxiesindividual objects: Lagoon nebula [ISM]StarsStar clusterAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary Astrophysics
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Gaia-ESO Survey: Gas dynamics in the Carina nebula through optical emission lines

2016

Aims. We present observations from the Gaia-ESO Survey in the lines of Hα, [N II], [S II], and He I of nebular emission in the central part of the Carina nebula. Methods. We investigate the properties of the two already known kinematic components (approaching and receding), which account for the bulk of emission. Moreover, we investigate the features of the much less known low-intensity high-velocity (absolute RV >50 km s) gas emission. Results. We show that gas giving rise to Hα and He I emission is dynamically well correlated with but not identical to gas seen through forbidden-line emission. Gas temperatures are derived from line-width ratios, and densities from [S II] doublet ratios. Th…

HII regionsastro-ph.SRastro-ph.GAAstrophysics::High Energy Astrophysical PhenomenaShell (structure)FluxFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesISM: individual objects: Carina nebula; ISM: general ; HII regionsIonization0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsHII regionEmission spectrum010303 astronomy & astrophysicsISM: individual objects: Carina nebulaQCSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsQBISM: generalAstronomía y AstrofísicaPhysicsNebulageneral [ISM]010308 nuclear & particles physicsindividual objects: Carina nebula [ISM]Astronomy and AstrophysicsGas dynamicsAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesDust laneCore (optical fiber)Astrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)HII regions; ISM: general; ISM: individual objects: Carina nebula; Astronomy and Astrophysics; Space and Planetary Science
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