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Lost in translation: Mystery of the missing text solved.Chaotic universe model.Alexander Friedmann and the origins of modern cosmologyHuman contrast threshold and astronomical visibilityEinstein’s conversion from his static to an expanding universeLXXXVI.On relativistic cosmologyThe origin and abundances of the chemical elementsStar-forming complexes and the spiral structure of our GalaxyEinstein’s 1917 static model of the universe: a centennial reviewThe dependence of the AV prior for SN Ia on host mass and disc inclinationGalaxy Zoo 2: detailed morphological classifications for 304 122 galaxies from the Sloan Digital Sky SurveyThe origin of discs and spheroids in simulated galaxiesThe Anatomy of GalaxiesSpiral galaxy distance indicators based on near-infrared photometryGalaxy Zoo: morphological classifications for 120 000 galaxies in HST legacy imagingGalaxy Zoo: quantitative visual morphological classifications for 48 000 galaxies from CANDELSARRAKIS: atlas of resonance rings as known in the S4GMorphological classification of local luminous infrared galaxiesGalaxy Zoo: quantifying morphological indicators of galaxy interaction★Galaxy and Mass Assembly (GAMA): formation and growth of elliptical galaxies in the group environmentDawes Review 4: Spiral Structures in Disc GalaxiesThe zCOSMOS 10k-sample: the role of galaxy stellar mass in the colour-density relation up toz ~ 1Cool dust heating and temperature mixing in nearby star-forming galaxiesThe SAMI Galaxy Survey: the link between angular momentum and optical morphologyGalaxy Zoo and sparcfire: constraints on spiral arm formation mechanisms from spiral arm number and pitch anglesGalaxy Zoo: comparing the demographics of spiral arm number and a new method for correcting redshift biasGalaxy Alignments: An OverviewGalaxy And Mass Assembly (GAMA): $\mathcal {M_\star }\text{--}R_{\rm e}$ relations ofz= 0 bulges, discs and spheroidsImplications and Applications of Kinematic Galaxy Scaling RelationsProperties of the Photometric Components of Lenticular GalaxiesGalaxy And Mass Assembly (GAMA): ugrizYJHK Sérsic luminosity functions and the cosmic spectral energy distribution by Hubble type1.65-μm (H-band) surface photometry of galaxies - VIII. The near-IRκspace atz=0The redshift and mass dependence on the formation of the Hubble sequence at z > 1 from CANDELS/UDSStructure through colour: a pixel approach towards understanding galaxiesH-ATLAS/GAMA: the nature and characteristics of optically red galaxies detected at submillimetre wavelengthsRadio AGN in spiral galaxiesThe importance of minor-merger-driven star formation and black hole growth in disc galaxiesThe significant contribution of minor mergers to the cosmic star formation budgetH-ATLAS/GAMA: quantifying the morphological evolution of the galaxy population using cosmic calorimetryVariations in 24-μm morphologies among galaxies in the Spitzer Infrared Nearby Galaxies Survey: new insights into the Hubble sequence
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P2860
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im Dezember 1926 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована в грудні 1926
@uk
name
Extragalactic nebulae
@en
Extragalactic nebulae
@nl
type
label
Extragalactic nebulae
@en
Extragalactic nebulae
@nl
prefLabel
Extragalactic nebulae
@en
Extragalactic nebulae
@nl
P356
P1476
Extragalactic nebulae
@en
P2093
E. P. Hubble
P304
P356
10.1086/143018
P407
P577
1926-12-01T00:00:00Z
P5875
P819
1926ApJ....64..321H