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The Mysterious Radcliffe Wave
DOI: 10.1007/s10511-023-09761-7 Bibcode: 2022Ap.....65..579B

Bobylev, V. V.; Bajkova, A. T.; Mishurov, Yu. N.

This survey is devoted to the Radcliffe Wave discovered recently by Alves et al., from an analysis of the position of molecular clouds. These authors identified a narrow chain of molecular clouds, extended essentially in one line at an angle of about 30° to the galactic axis y. Essentially, the Radcliffe Wave outlines the damped oscillations in th…

2022 Astrophysics
Gaia 3
Analysis of Emission Line Widths of [CII] 158µm
DOI: 10.1007/s10511-022-09728-0 Bibcode: 2022Ap.....65..151S

Samsonyan, A. L.

A study of [CII] 158 µm emission line profiles observed with Herschel PACS for 379 galaxies is presented. Emission line widths are compared to [CII] luminosities, to near-infrared 1.6 µm luminosities and to infrared 22 µm luminosities to decide if any luminosity relates to velocity dispersion. Archival data for [CII] fluxes and l…

2022 Astrophysics
Herschel 1
Spottedness Activity of the Young Star HIP 94235 from the Moving Group AB Doradus
DOI: 10.1007/s10511-023-09765-3 Bibcode: 2022Ap.....65..512S

Savanov, I. S.

Based on high-precision data from the archive of the TESS space mission, a study is made of the photometric variability of the brightness of HIP 94235, a bright star belonging to the 120 million years old moving group AB Doradus. We obtained an estimate for the rotation period of the star and the amplitude of the brightness variability, as well as…

2022 Astrophysics
Gaia 0