Results 91 to 100 of about 151,849 (119)

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]

Lenticular 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.
Graham, Alister W.
core  

Phenomenological analysis of observed relations for low-redshift galaxies. [PDF]

Proc Natl Acad Sci U S A, 1975
Nicoll JF, Segal IE.
europepmc   +1 more source

Unsupervised multimodal deep learning for galaxy morphology taxonomy: integrating ConvNeXtEmbeddings and morphological parameters for scalable survey science. [PDF]

Sci Rep
Selim IM, Farahat AS, Basmsm LH, El-Hameed AMA.   +3 more
europepmc   +1 more source

The Surface Brightness Fluctuations and Globular Cluster Populations of Virgo Elliptical and Lenticular Galaxies

, 1999
The Virgo cluster of galaxies is a complex system composed of several subclusters or "clouds." Although the relative positions of clouds can be determined by the low precision measurement of many galaxies in each cloud, the internal structure ...
Eric H. Neilsen, By Eric Neilsen
core  

A rising tide: intrinsic alignments since the turn of the millennium. [PDF]

Astron Astrophys Rev
Chisari NE.
europepmc   +1 more source

Calculation of Extra Curve of Negative Lenticular Spectacle Lenses

, 1985
Lenticular designs are useful for high negative spectacle prescriptions. This paper presents an accurate method for determining the power of the extra curve to be surfaced on the back surfaces of a negative lenticular spectacle lens in order to obtain ...
Atchison, David A.
core  

Strong Lensing by Galaxies. [PDF]

Space Sci Rev
Shajib AJ, Vernardos G, Collett TE, Motta V, Sluse D, Williams LLR, Saha P, Birrer S, Spiniello C, Treu T.   +9 more
europepmc   +1 more source

No-rank tensor decomposition via metric learning. [PDF]

Sci Rep
Bagherian M.
europepmc   +1 more source

Newly formed dust within the circumstellar environment of SN Ia-CSM 2018evt. [PDF]

Nat Astron
Wang王 L灵, Hu M, Wang L, Yang 杨 Y轶, Yang J, Gomez H, Chen S, Hu L, Chen TW, Mo J, Wang X, Baade D, Hoeflich P, Wheeler JC, Pignata G, Burke J, Hiramatsu D, Howell DA, McCully C, Pellegrino C, Galbany L, Hsiao EY, Sand DJ, Zhang J, Uddin SA, Anderson JP, Ashall C, Cheng C, Gromadzki M, Inserra C, Lin H, Morrell N, Morales-Garoffolo A, Müller-Bravo TE, Nicholl M, Gonzalez EP, Phillips MM, Pineda-García J, Sai H, Smith M, Shahbandeh M, Srivastav S, Stritzinger MD, Yang S, Young DR, Yu L, Zhang X.   +46 more
europepmc   +1 more source

Cambridge Cosmology: Galaxies

This section of Cambridge Cosmology explores the topic of galaxies. It discusses statistics and parts of our own galaxy, the Milky Way, as well as other classes of galaxies (spiral, elliptical, lenticular, and irregular).
Paul Shellard, Jiun-Huei Wu
core