Showing 1–20 of 32 results
/ Date/ Name
Sep 28, 2021Stellar Population Astrophysics (SPA) with the TNG: Stock 2, a little-studied open cluster with an eMSTOFeb 12, 2024TOI-1199 b and TOI-1273 b: Two new transiting hot Saturns detected and characterized with SOPHIE and TESSApr 26, 2024Cepheid Metallicity in the Leavitt Law (C- MetaLL) survey: VI: Radial abundance gradients of 29 chemical species in the Milky Way DiskApr 5, 2017NGC 6067: a young and massive open cluster with high metallicityFeb 15, 2022Proton acceleration in thermonuclear nova explosions revealed by gamma raysApr 24, 2026The circumstellar environment of the young, low-mass dipper star JH 223. Accretion and large-scale magnetic field topologyFeb 26, 2024TESS photometry and CAOS spectroscopy of six eclipsing binaries with Am componentsJan 31, 2023Stable accretion and episodic outflows in the young transition disk system GM AurigaeMay 25, 2022The multichord stellar occultation on 2019 October 22 by the trans-Neptunian object (84922) 2003 VS$_2$Sep 11, 2019A comprehensive study of NGC 2345, a young open cluster with a low metallicityJan 17, 2022The ODYSSEUS Survey. Motivation and First Results: Accretion, Ejection, and Disk Irradiation of CVSO 109Oct 18, 2024The Radcliffe Wave as traced by young open clusters: Stellar parameters, activity indicators, and abundances of solar-type members of eight young clustersJul 20, 2025Stellar Population Astrophysics (SPA) with the TNG: NLTE atmospheric parameters and abundances of giant stars in 33 Open ClustersSep 25, 2020Three open clusters containing Cepheids: NGC 6649, NGC 6664 and Berkeley 55Sep 13, 2021PENELLOPE II. CVSO 104: a pre-main sequence close binary with an optical companion in Ori OB1Dec 14, 2023High-resolution spectroscopy of the young open cluster M 39 (NGC 7092)Apr 27, 2015The little-studied cluster Berkeley 90. I. LS III +46 11: a very massive O3.5 If* + O3.5 If* binaryApr 12, 2025LAMOST medium-resolution observations of the PleiadesApr 13, 2026NGC 1647: A young open cluster with a broad main sequence observed with LAMOSTJul 1, 2022New, late-type spectroscopic binaries with X-ray emission