On the Origin of the 107 K Hot Emitting Gas in the Circumgalactic Medium of the Milky Way
The presence of the ≈10 ^6 K gas in the circumgalactic medium of the Milky Way (MW) has been well established. However, the location and the origin of the newly discovered hot gas at “supervirial (SV)” temperatures of ≈10 ^7 K have been puzzling.
Mukesh Singh Bisht+2 more
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An SDSS Sky Survey for Resolved Milky Way Satellite Galaxies. II. High-Velocity Clouds in the Early Data Release [PDF]
Beth Willman+4 more
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Predicting Interstellar Object Chemodynamics with Gaia
The interstellar object (ISO) population of the Milky Way is a product of its stars. However, what is in fact a complex structure in the solar neighborhood has traditionally in ISO studies been described as smoothly distributed.
Matthew J. Hopkins+2 more
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A Catalog of Distance Determinations for 5 Million Stars in LAMOST DR10
Using the distance estimation method outlined in J. L. Carlin et al., a Bayesian approach specifically tailored for LAMOST data, we estimated distances for 7,450,303 spectra from 5,394,174 unique stars in the LAMOST DR10 low-resolution data set.
Chengqun Yang+5 more
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Under the assumption of a simple and time-invariant gravitational potential, many Galactic dynamics techniques infer the milky Way’s mass and dark matter distributions from stellar kinematic observations.
Danny Horta+7 more
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The Extremely Metal-rich Knot of Stars at the Heart of the Galaxy
We show with Gaia XP spectroscopy that extremely metal-rich (EMR) stars in the Milky Way ([M/H] _XP ≳ 0.5) are largely confined to a tight “knot” at the center of the Galaxy. This EMR knot is round in projection, has a fairly abrupt edge near R _GC,proj ∼
Hans-Walter Rix+17 more
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Observations of magnetic fields in the Milky Way and in nearby galaxies with a Square Kilometre Array [PDF]
R. Beck, B. M. Gaensler
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Radial Wave in the Galactic Disk: New Clues to Discriminate Different Perturbations
Decoding the key dynamical processes that shape the Galactic disk structure is crucial for reconstructing the Milky Way’s evolution history. The second Gaia data release unveils a novel wave pattern in the L _Z −〈 V _R 〉 space, but its formation ...
Chengye Cao+3 more
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Is the Dust Obscuring Supernovae in Distant Galaxies the Same as Dust in the Milky Way?
Adam G. Riess+2 more
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A dwarf galaxy remnant in Canis Major: the fossil of an in-plane accretion on to the Milky Way [PDF]
Nicolas F. Martin+5 more
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