Results 131 to 140 of about 106,694 (288)
We predict the sensitivity of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) to faint, resolved Milky Way satellite galaxies and outer-halo star clusters.
Kabelo Tsiane +10 more
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Galaxies Behind the Milky Way and the Great Attractor [PDF]
Lecture Series presented at the Mexican School of Astrophysics in Guanajuato, August 1999. In press in the series "Lecture Notes in Physics: GTO Lectures on Astrophysics", eds. D. Page and J. Hirsch, Springer: Heidelberg, p301-344, 18 figures, uses various included stylefiles. Version with full resolution available upon request (kraan@astro.ugto.mx)
openaire +3 more sources
Redshift Distribution of Galaxies in the Southern Milky way Region 210° < I < 360° and |b| < 15° [PDF]
Natarajan Vivanathan, Tōru Yamada
openalex +1 more source
Gas Transfer between the Inner 3 kpc Disk and the Galactic Central Molecular Zone
We uncovered a more tilted molecular gas structure with highly negative velocities located near the dust lane. Our observations show that the approaching gas flows from the overshoot process are captured by the gravitational potential of the bar and then
Yang Su +12 more
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Astronomically, the Milky Way is a big star system _ a galaxy. The word galaxy is derived from the Greek gala `milk'. In many languages the Milky Way's name is connected with milk. However, in Estonia this form of the name is rare.
Andres Kuperjanov
doaj
Revealing Gas Inflows Toward the Galactic Central Molecular Zone
We study the gas inflows toward the Galactic Central Molecular Zone (CMZ) based on the gas morphological and kinematic features from the Milky Way Imaging Scroll Painting in the region of l = 1.°2–19.°0 and ∣ b ∣ ≲ 3.°0.
Yang Su +9 more
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A Visual Search for Galaxies in a Milky Way Region around the North Supergalactic Pole [PDF]
A. T. Roman, Ikuru Iwata, Mamoru Saitō
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A Wave-corrected Assessment of the Local Midplane
As the number of known Galactic structures mounts thanks to the Gaia Space Telescope, it is now pertinent to study methods for disentangling structures occupying the same regions of the Milky Way. Indeed, understanding the precise form of each individual
Ziyuan Yin, Austin Hinkel
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We present an analysis of the structure, kinematics, and chemo-dynamical properties of the Milky Way bulge using RR Lyrae stars from Optical Gravitational Lensing Experiment (OGLE), and giant stars from APOGEE and Gaia that have distances placing them in
Xiao Han +7 more
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Are dSph galaxies Galactic building blocks?
Dwarf spheroidal galaxies (dSph) are frequently assumed to represent surviving examples of a vast now destroyed population of small systems in which many of the stars now forming the Milky Way were formed. Ongoing accretion and considerable sub-structure
Gilmore G., Asiri H.M.
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