Results 141 to 150 of about 406 (178)

Multiomic profiling of medulloblastoma reveals subtype-specific targetable alterations at the proteome and N-glycan level. [PDF]

Nat Commun
Godbole S, Voß H, Gocke A, Schlumbohm S, Schumann Y, Peng B, Mynarek M, Rutkowski S, Dottermusch M, Dorostkar MM, Korshunov A, Mair T, Pfister SM, Kwiatkowski M, Hotze M, Neumann P, Hartmann C, Weis J, Liesche-Starnecker F, Guan Y, Moritz M, Siebels B, Struve N, Schlüter H, Schüller U, Krisp C, Neumann JE.   +26 more
europepmc   +1 more source

Unraveling the role of cloud computing in health care system and biomedical sciences. [PDF]

Heliyon
Sachdeva S, Bhatia S, Al Harrasi A, Shah YA, Anwer K, Philip AK, Shah SFA, Khan A, Ahsan Halim S.   +8 more
europepmc   +1 more source

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The Andromeda Galaxy

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
exaly   +2 more sources

Neutral Hydrogen Survey of Andromeda Galaxy

Science, 1966
A 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
exaly   +3 more sources

Observations of the Andromeda Galaxy at 11-Centimeter Wavelength

Science, 1967
Observations 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
exaly   +3 more sources

The andromeda galaxy M31

Astrophysics, 1972
exaly   +2 more sources

The andromeda galaxy M 31

Astrophysics, 1970
exaly   +2 more sources

The Andromeda Galaxy

Scientific American, 1981
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.
openaire   +1 more source

Radio Map of the Andromeda Galaxy

Science, 1964
The University of Illinois radio telescope has resolved the 610.5 Mcy/sec disk component of radio emission from the large galaxy M 31 into several discrete concentrations. In two cases, these correspond to the crossing of the optical major axis by spiral arms. A spur of emission extends southeast from the galaxy near the minor axis.
openaire   +2 more sources

Methanol Masers in the Andromeda Galaxy

Proceedings of the International Astronomical Union, 2017
AbstractIs M31 going to collide with the Milky Way, or spiral around it? Determining the gravitational potential in the Local Group has been a challenge since it requires 3D space velocities and orbits of the members, and most objects have only had line-of-sight velocities measured. Compared to the less massive group members, the transverse velocity of
Ylva M. Pihlström, Loránt O. Sjouwerman   +1 more
openaire   +1 more source