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Transformation of the equatorial proper motion to the Galactic system

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arxiv 1306.2945 v3 pith:GX7WLLUU submitted 2013-06-12 astro-ph.IM

classification astro-ph.IM
keywords equatorialgalacticmotionproperanalyticalcoordinatesequationssimple
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I present simple analytical equations to transform proper motion vectors from equatorial to Galactic coordinates.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Dynamical mass distribution and velocity structure of the Galactic centre

    astro-ph.GA 2025-06 conditional novelty 6.0 of 10

    Dynamical models of 4,600 Galactic centre stars give a black hole mass of 4.35 million solar masses and a mass profile that is lower than earlier work by up to roughly 75% at 15 pc.

  2. The evolution of velocity dispersion in the Sco-Cen OB association

    astro-ph.GA 2025-09 unverdicted novelty 5.0 of 10

    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.

  3. 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

    astro-ph.GA 2026-05 unverdicted novelty 4.0 of 10

    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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