Results 251 to 260 of about 12,683,757 (268)
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Resolving the hot and ionized Universe through the Sunyaev-Zeldovich effect. [PDF]
Di Mascolo L+24 more
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Distraction Therapies for Office-Based Otolaryngology Procedures Performed on the Upper Airway. [PDF]
Curry T, Lasso A, Kilty S.
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Suicidal risk is associated with hyper-connections in the frontal-parietal network in patients with depression. [PDF]
Ren Y+13 more
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DANTE and DANTE_LTR: lineage-centric annotation pipelines for long terminal repeat retrotransposons in plant genomes. [PDF]
Novák P+3 more
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Enhanced sensitivity of TAPscan v4 enables comprehensive analysis of streptophyte transcription factor evolution. [PDF]
Petroll R+6 more
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HIBRID: Histology and ct-DNA based Risk-stratification with Deep Learning
Loeffler CM+23 more
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2000
Before stellar evolution theory reached its present stage, galactic evolution ideas were tentative and depended not so much on physical arguments (e.g. galactic dynamics) but intuitive notions based on observations of galaxy shapes. Historically this is quite understandable.
Michael Stecker, Bernard Abrams
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Before stellar evolution theory reached its present stage, galactic evolution ideas were tentative and depended not so much on physical arguments (e.g. galactic dynamics) but intuitive notions based on observations of galaxy shapes. Historically this is quite understandable.
Michael Stecker, Bernard Abrams
openaire +2 more sources
2004
Few galaxies are loners: almost all are members of groups of at least a dozen systems. The Milky Way is no exception. It is the second brightest in a group of three dozen, mostly dwarf, galaxies. The brightest member of the Local Galaxy Group is the Andromeda Spiral M31. The most luminous members of the Local Group, including all those visible with any
Craig Crossen, Gerald Rhemann
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Few galaxies are loners: almost all are members of groups of at least a dozen systems. The Milky Way is no exception. It is the second brightest in a group of three dozen, mostly dwarf, galaxies. The brightest member of the Local Galaxy Group is the Andromeda Spiral M31. The most luminous members of the Local Group, including all those visible with any
Craig Crossen, Gerald Rhemann
openaire +2 more sources
Dwarf Galaxies in Nearby Groups of Galaxies [PDF]
We have confirmed 19 new dwarf members in five nearby (z ≤ 0.014) groups of galaxies, measured their photometric characteristics and compared the photometric scaling relations of the late-type dwarf galaxies in the field, group and cluster environments.
Ulrich Hopp, J. Vennik
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