Results 121 to 130 of about 10,527 (159)
EBIT Observation of Ar Dielectronic Recombination Lines near the Unknown Faint X-Ray Feature Found in the Stacked Spectrum of Galaxy Clusters. [PDF]
Gall AC +9 more
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Interactors and effects of overexpressing YlxR/RnpM, a conserved RNA binding protein in cyanobacteria. [PDF]
Hemm L +8 more
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Multiomic profiling of medulloblastoma reveals subtype-specific targetable alterations at the proteome and N-glycan level. [PDF]
Godbole S +26 more
europepmc +1 more source
Uncovering the non-histone interactome of the BRPF1 bromodomain using site-specific azide-acetyllysine photochemistry. [PDF]
Barman S, Padhan J, Sudhamalla B.
europepmc +1 more source
Unraveling the role of cloud computing in health care system and biomedical sciences. [PDF]
Sachdeva S +8 more
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Astrophysics and Space Science Library, 1992
1. Early History.- 2. Discovery of its Galaxian Nature.- 3. Modern History.- 4. Optical Structure.- 5. The Neutral Hydrogen Content.- 6. Radio Continuum Radiation.- 7. Rotation.- 8. Dynamics and Mass.- 9. Globular Clusters.- 10. OB Associations.- 11. Open Clusters.- 12. Dust.- 13. Variable Stars and Novae.- 14.
Paul Hodge
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1. Early History.- 2. Discovery of its Galaxian Nature.- 3. Modern History.- 4. Optical Structure.- 5. The Neutral Hydrogen Content.- 6. Radio Continuum Radiation.- 7. Rotation.- 8. Dynamics and Mass.- 9. Globular Clusters.- 10. OB Associations.- 11. Open Clusters.- 12. Dust.- 13. Variable Stars and Novae.- 14.
Paul Hodge
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Neutral Hydrogen Survey of Andromeda Galaxy
Science, 1966A neutral hydrogen survey of the Andromeda galaxy (M31) has been conducted with the 260-foot (80m) Ohio State University radio telescope. The neutral hydrogen is concentrated in the spiral arm regions, with but relatively small amounts near the center of the galaxy.
W D, Brundage, J D, Kraus
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Observations of the Andromeda Galaxy at 11-Centimeter Wavelength
Science, 1967Observations of the Andromeda galaxy (M31) at 2695 megahertz reveal more detail than do earlier measurements at lower frequency. The region is highly confused but there is apparently a more dense clustering of sources within the optical outline of the galaxy than without. One source (OA33) near M31 has an interesting, flat spectrum.
G W Swenson
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