A nearby dark molecular cloud in the Local Bubble revealed via H<sub>2</sub> fluorescence. [PDF]
Burkhart B +22 more
europepmc +1 more source
Long-term effects of combined exposures to simulated microgravity and galactic cosmic radiation on the mouse lung: sex-specific epigenetic reprogramming. [PDF]
Clement K +11 more
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Milky Way could invalidate the hypothesis of exotic matter and favor a gravitomagnetic solution to explain dark matter. [PDF]
Le Corre S.
europepmc +1 more source
Reverberation lags viewed in hard X-rays from an accreting stellar-mass black hole. [PDF]
You B +7 more
europepmc +1 more source
Discovery of a high-velocity cloud of the Milky Way as a potential dark galaxy. [PDF]
Liu XL +8 more
europepmc +1 more source
Nonequilibrium Synthesis of Glycolamide (NH<sub>2</sub>COCH<sub>2</sub>OH), a Precursor to Amino Acids, on Interstellar Nanoparticles. [PDF]
Bergantini A +5 more
europepmc +1 more source
Galaxy Tomography with the Gravitational Wave Background from Supermassive Black Hole Binaries
Chen Y.
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ABSTRACTThe Galactic center is a superb laboratory of modern astrophysics where astronomers can study at unprecedented spatial resolution and across the entire electromagnetic spectrum physical processes that may also happen at the cores of other galaxies. Following a brief review of the phenomena observed in the central few hundred parsecs, we discuss
R. Genzel, A. Eckart, A. Krabbe
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The Galactic Center large program
AIP Conference Proceedings, 2008We report a multi‐epoch and multi‐wavelength observation campaign of the Galactic Center. Some results are first presented before stressing more specifically the 8.6 micron observations obtained with VLT/VISIR used in burst mode during three nights in July 2007.
X. Haubois +9 more
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A brief review of galactic center observations, from the radio to gamma rays, is presented. There is evidence for black holes in the central region of the Galaxy at all wavelengths, but the observations are not unambiguous and a single massive object at the dynamic center may not explain the data at all wavelengths. Requirements for future observations
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