Distance determination for RAVE stars using stellar models II: Most
likely values assuming a standard stellar evolution scenario

Distance determination for RAVE stars using stellar models II: Most likely values assuming a standard stellar evolution scenario

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The RAdial Velocity Experiment (RAVE) is a spectroscopic survey of the Milky Way. We use the subsample of spectra with spectroscopically determined values of stellar parameters to determine the distances to these stars. The list currently contains 235,064 high quality spectra which show no peculiari...

Deskribapen osoa

Xehetasun bibliografikoak
Egile Nagusiak:	Zwitter, T, vc, G, Breddels, M, Smith, M, Helmi, A, Munari, U, Bienaymé, O, Binney, J, Bland-Hawthorn, J, Boeche, C, Brown, A, Campbell, R, Freeman, K, Fulbright, J, Gibson, B, Gilmore, G, Grebel, E, Navarro, J, Parker, Q, Seabroke, G, Siebert, A, Siviero, A, Steinmetz, M, Watson, F, Williams, M
Formatua:	Journal article
Hizkuntza:	English
Argitaratua:	2010

Antzeko izenburuak

Distance determination for RAVE stars using stellar models: II. Most likely values assuming a standard stellar evolution scenario
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Distance determination for RAVE stars using stellar models
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Distance determination for RAVE stars using stellar models
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Distance determination for RAVE stars using stellar models
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Distance determination for RAVE stars using stellar models III. The nature of the RAVE survey and Milky Way chemistry
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Distance determination for RAVE stars using stellar models III: The nature of the RAVE survey and Milky Way chemistry
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KINEMATIC MODELING OF THE MILKY WAY USING THE RAVE AND GCS STELLAR SURVEYS
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Estimation of the Tilt of the Stellar Velocity Ellipsoid from RAVE and Implications for Mass Models
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Is the sky falling? Searching for stellar streams in the local Milky Way disc in the CORAVEL and RAVE surveys
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Testing formation mechanisms of the Milky Way's thick disc with RAVE
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Testing formation mechanisms of the Milky Way's thick disc with RAVE
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In the thick of it: metal-poor disc stars in RAVE
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The Dawning of the Stream of Aquarius in RAVE
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Galactic kinematics with RAVE data
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THE DAWNING OF THE STREAM OF AQUARIUS IN RAVE
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RAVE spectroscopy of luminous blue variables in the Large Magellanic Cloud
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RAVE spectroscopy of luminous blue variables in the Large Magellanic Cloud
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The RAVE Survey: Rich in Very Metal-Poor Stars
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The RAVE survey: Rich in very metal-poor stars
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THE RAVE SURVEY: RICH IN VERY METAL-POOR STARS
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Chemical separation of disc components using RAVE
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Diffuse interstellar bands in RAVE Survey spectra
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The RAVE Survey: Constraining the Local Galactic Escape Speed
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The properties of the local spiral arms from RAVE data: two-dimensional density wave approach
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Chemical gradients in the Milky Way from the RAVE data. I. Dwarf stars
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New distances to RAVE stars
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Origins of the thick disk as traced by the alpha elements of metal-poor giant stars selected from RAVE
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ORIGINS OF THE THICK DISK AS TRACED BY THE ALPHA ELEMENTS OF METAL-POOR GIANT STARS SELECTED FROM RAVE
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Origins of the Thick Disk as Traced by the Alpha-Elements of Metal-Poor Giant Stars Selected from RAVE
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Detection of a radial velocity gradient in the extended local disc with RAVE
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Detection of a radial velocity gradient in the extended local disc with RAVE
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Galactic kinematics with RAVE data: I. The distribution of stars towards the Galactic poles
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The Radial Velocity Experiment (RAVE): second data release
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The selection function of the RAVE survey
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Galactic kinematics and dynamics from RAVE stars
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Constraining the Galaxy's dark halo with RAVE stars
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The RAVE survey: the Galactic escape speed and the mass of the Milky Way
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The wobbly Galaxy: kinematics north and south with RAVE red-clump giants
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DIFFUSE INTERSTELLAR BAND AT 8620 angstrom IN RAVE: A NEW METHOD FOR DETECTING THE DIFFUSE INTERSTELLAR BAND IN SPECTRA OF COOL STAR
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Chemical gradients in the Milky Way from the RAVE data. II. Giant stars
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