{ "id": "1902.09569", "version": "v1", "published": "2019-02-25T19:09:11.000Z", "updated": "2019-02-25T19:09:11.000Z", "title": "More than just a wrinkle: A wave-like pattern in radial velocity vs. angular momentum from Gaia Data", "authors": [ "Jennifer Friske", "Ralph Schönrich" ], "comment": "10 pages, 12 figures, submitted to MNRAS", "categories": [ "astro-ph.GA" ], "abstract": "We present a newly found wave--like pattern in mean Galactocentric radial velocity U_g vs. guiding centre radius R_g or angular momentum L_z of stars in the RV subsample of Gaia DR2. The short-wave pattern has a wavelength of order 1.2 kpc in R_g or 285 kpc km/s in L_z. The pattern shows only weak changes with Galactocentric radius R and little change in strength in particular with the vertical energy E_z of the stars or respectively the distance to the Galactic plane |z|. The pattern is to first order symmetric around the plane, i.e. has no significant odd terms in z. There is weak phase shift with the pattern moving towards slightly lower L_z (i.e. trailing) with |z| and E_z. However, we observe a highly significant phase shift in Galactic azimuth phi, which is different for different peaks. The peak around L_z ~ 2100 kpc km/s shows weak/uncertain change and shifts by of order dL_z/d phi ~ (97 +/- 32) kpc km/s/rad, while the rest of the pattern shows a clearly detectable shift of ~ (200 +/- 22) kpc km/s/rad. If we consider all peaks to belong to the same pattern, this would suggest a wavenumber m = 4. We further find that the wave-like pattern in U_g appears to be related to the W vs. L_z pattern detected in Gaia DR1. A comparison of the U_g-L_z wave pattern with changes of U_g vs. R, which have been previously discussed, suggests that the latter can be understood as just the U_g-L_z pattern washed out by blurring (i.e. orbital excursions around their guiding-centre) of disc stars.", "revisions": [ { "version": "v1", "updated": "2019-02-25T19:09:11.000Z" } ], "analyses": { "keywords": [ "angular momentum", "wave-like pattern", "gaia data", "kpc km/s/rad", "mean galactocentric radial velocity" ], "note": { "typesetting": "TeX", "pages": 10, "language": "en", "license": "arXiv", "status": "editable" } } }