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2024RAA....24c5010B - Research in Astron. and astroph., 24, part no 3, 5010 (2024/March-0)

The Radcliffe Wave Parameters from Data on Open Star Clusters.

BOBYLEV V.V. and BAJKOVA A.T.

Abstract (from CDS):

A spectral analysis of the vertical positions and velocities of 374 open star clusters (OSCs) was carried out. We took these OSCs from the Hunt and Reffert catalog; they have an average age of about 10 million years, and are located on the galactic plane XY in a narrow zone inclined by 25° to the galactic axis Y. The following estimates of the parameters of the Radcliffe wave were obtained: (a) the maximum value in periodic perturbations of vertical coordinates ${Z}_{\max }=92\pm 10$ pc with the wavelength of these perturbations λz = 4.82 ± 0.09 kpc; (b) the maximum value of the velocity of vertical disturbances ${W}_{\max }=4.36\pm 0.12$ km s–1 with disturbance wavelength λW = 1.78 ± 0.02 kpc. Note that the results of the vertical velocity analysis are first-class in accuracy and completely new.

Abstract Copyright: © 2024 National Astronomical Observatories

Journal keyword(s): (Galaxy:) local interstellar matter - Galaxy: structure - (Galaxy:) solar neighborhood

Simbad objects: 4

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