Results 161 to 170 of about 10,594 (212)

Young Accreting Compact Objects in M31: The Combined Power of <i>NuSTAR, Chandra</i>, and <i>Hubble</i>. [PDF]

open access: yesAstrophys J, 2018
Lazzarini M   +13 more
europepmc   +1 more source

EBIT Observation of Ar Dielectronic Recombination Lines near the Unknown Faint X-Ray Feature Found in the Stacked Spectrum of Galaxy Clusters. [PDF]

open access: yesAstrophys J, 2019
Gall AC   +9 more
europepmc   +1 more source

Interactors and effects of overexpressing YlxR/RnpM, a conserved RNA binding protein in cyanobacteria. [PDF]

open access: yesRNA Biol
Hemm L   +8 more
europepmc   +1 more source

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

open access: yesNat Commun
Godbole S   +26 more
europepmc   +1 more source

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

open access: yesHeliyon
Sachdeva S   +8 more
europepmc   +1 more source

AVJ16 inhibits lung carcinoma by targeting IGF2BP1. [PDF]

open access: yesOncogene
Wallis N   +10 more
europepmc   +1 more source

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
openaire   +4 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

AGAPE, Andromeda galaxy and amplified pixels experiment

Nuclear Physics B - Proceedings Supplements, 1995
The galaxy M31 is a very good potential target for microlensing searches. However, only few stars are resolved, and a different method is therefore needed : monitor pixels and not stars. This method, and the AGAPE project based on it, are presented here.
Ansari, R.   +13 more
openaire   +2 more sources

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