Evolution of asymptotic giant branch stars - II. Optical to far-infrared isochrones with improved TP-AGB models
A&A, 482 3 (2008) 883-905
Published online: 2008-03-04
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A NEWLY RECOGNIZED VERY YOUNG SUPERNOVA REMNANT IN M83,,
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Complex Stellar System ESO65SC03: Open Cluster or Remnant?
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THE PANCHROMATICHUBBLEANDROMEDA TREASURY. XI. THE SPATIALLY RESOLVED RECENT STAR FORMATION HISTORY OF M31
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Biases in the determination of dynamical parameters of star clusters: today and in the Gaia era
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THE NON-UNIVERSALITY OF THE LOW-MASS END OF THE IMF IS ROBUST AGAINST THE CHOICE OF SSP MODEL
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MEASURING INFRARED SURFACE BRIGHTNESS FLUCTUATION DISTANCES WITHHSTWFC3: CALIBRATION AND ADVICE
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ASTEROSEISMIC ESTIMATE OF HELIUM ABUNDANCE OF A SOLAR ANALOG BINARY SYSTEM
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PPMXL PHOTOMETRIC STUDY OF FOUR OPEN CLUSTER CANDIDATES (IVANOV 2, IVANOV 7, IVANOV 9 AND HARVARD 9)
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The VLT-FLAMES Tarantula Survey. XV. VFTS 822: A candidate Herbig B[e] star at low metallicity
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Photometric study of the open cluster – II. Stellar population and dynamical evolution in NGC 559
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THE CORE MASS GROWTH AND STELLAR LIFETIME OF THERMALLY PULSING ASYMPTOTIC GIANT BRANCH STARS
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A systematic look at the effects of radiative feedback on disc galaxy formation
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OPTICAL OBSERVATIONS OF THE TYPE Ic SUPERNOVA 2007gr IN NGC 1058
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Investigation of the stellar content in the western part of the Carina nebula
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