0000000001306665

AUTHOR

R. Szczerba

showing 2 related works from this author

Validating post-AGB candidates in the LMC and SMC using SALT spectra

2020

We selected a sample of post-AGB candidates in the Magellanic Clouds on the basis of their near- and mid-infrared colour characteristics. Fifteen of the most optically bright post-AGB candidates were observed with the South African Large Telescope in order to determine their stellar parameters and thus to validate or discriminate their nature as post-AGB objects in the Magellanic Clouds. The spectral types of absorption-line objects were estimated according to the MK classification, and effective temperatures were obtained by means of stellar atmosphere modelling. Emission-line objects were classified on the basis of the fluxes of the emission lines and the presence of the continuum. Out of…

Physics010308 nuclear & particles physicsYoung stellar objectContinuum (design consultancy)Stellar atmosphereFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsStellar classificationAstrophysics - Astrophysics of Galaxies01 natural sciencesPlanetary nebulaPhotometry (optics)StarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencesEmission spectrum010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astronomy & Astrophysics
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Post-AGB candidates in LMC and SMC SALT spectra

2020

We selected a sample of post-AGB candidates in the Magellanic Clouds on the basis of their near- and mid-infrared colour characteristics. Fifteen of the most optically bright post-AGB candidates were observed with the South African Large Telescope in order to determine their stellar parameters and thus to validate or discriminate their nature as post-AGB objects in the Magellanic Clouds. The spectral types of absorption-line objects were estimated according to the MK classification, and effective temperatures were obtained by means of stellar atmosphere modelling. Emission-line objects were classified on the basis of the fluxes of the emission lines and the presence of the continuum. Out of…

observational astronomygalactic and extragalactic astronomyAstrophysics and AstronomyStellar AstronomyPhysicsGiant starsMagellanic CloudsNatural SciencesSpectroscopy
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