Sco-Cen shows abrupt jumps and plateaus in velocity dispersion correlated with star formation bursts, indicating isotropic expansion, inside-out propagation at 5-6 km/s, and stellar feedback as the primary driver.
Transformation of the equatorial proper motion to the Galactic system
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abstract
I present simple analytical equations to transform proper motion vectors from equatorial to Galactic coordinates.
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Five new open clusters found via Gaia DR3 clustering and multiwavelength checks indicate an intrinsic low-density star-formation node in the Carina-Sagittarius Arm rather than extinction.
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The evolution of velocity dispersion in the Sco-Cen OB association
Sco-Cen shows abrupt jumps and plateaus in velocity dispersion correlated with star formation bursts, indicating isotropic expansion, inside-out propagation at 5-6 km/s, and stellar feedback as the primary driver.
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Multiwavelength study of the Carina--Sagittarius Arm. I.Astrometric and photometric search for new open clusters in the 320$^ \circ $ $\le$ l $\le$ 325$^ \circ $ region
Five new open clusters found via Gaia DR3 clustering and multiwavelength checks indicate an intrinsic low-density star-formation node in the Carina-Sagittarius Arm rather than extinction.