Knowledge-enhanced prototypical network with class cluster loss for few-shot relation classification. [PDF]
PLoS One, 2023 Liu T, Ke Z, Li Y, Silamu W.
europepmc +1 more source
Young Stellar Nuclei in the Lenticular Galaxies. II. NGC 7280 [PDF]
, 2000 V. L. Afanasiev +1 more
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Young Stellar Nuclei in Lenticular Galaxies: NGC 5574 and NGC 7457 [PDF]
, 2002 О. К. Сильченко +3 more
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Precision Landing of a Quadcopter Drone by Smartphone Video Guidance Sensor in a GPS-Denied Environment. [PDF]
Sensors (Basel), 2023 Bautista N +3 more
europepmc +1 more source
Uses, Botanical Characteristics, and Phenological Development of Slender Nightshade (Solanum nigrescens Mart. and Gal.). [PDF]
Plants (Basel), 2023 Ramírez-Olvera SM, Sandoval-Villa M.
europepmc +1 more source
Stellar population properties in the nuclei and bulges of nearby lenticular galaxies [PDF]
, 2004 О. К. Сильченко
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Clues to the Formation of Lenticular Galaxies Using Spectroscopic Bulge-Disk Decomposition [PDF]
arXiv, 2013 Lenticular galaxies have long been thought of as evolved spirals, but the processes involved to quench the star formation are still unclear. By studying the individual star formation histories of the bulges and disks of lenticulars, it is possible to look for clues to the processes that triggered their transformation from spirals.
arxiv
The SAURON project – VIII. OASIS/CFHT integral-field spectroscopy of elliptical and lenticular galaxy centres* [PDF]
, 2006 Richard M. McDermid +12 more
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The H I content of elliptical and lenticular galaxies withrecent star formation [PDF]
, 2007 J. F. Helmboldt
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Repainting the colour-mass diagrams by unearthing the green mountain: dust-rich S0 galaxies in the colour-(galaxy stellar mass) diagram, and the colour-(black hole mass) relations for dust-poor versus dust-rich galaxies [PDF]
arXivLenticular galaxies are notoriously misclassified as elliptical galaxies and, as such, a (disc inclination)-dependent correction for dust is often not applied to the magnitudes of dusty lenticular galaxies. This results in overly red galaxy colours, impacting their distribution in the colour-magnitude diagram.
arxiv