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20232026
most citedThe GALAH survey: Tracing the Milky Way's formation and evolution through RR Lyrae stars

20 citations · 30 across the 9 of their papers we have counts for

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6 papers · 1 filter

astro-ph.SR2026

On the use of field RR Lyrae as Galactic probes:. IX. Radial velocities

K. Baeza-Villagra, V. F. Braga, M. Fabrizio +25

We present the largest and most homogeneous catalog of radial velocity (RV) measurements for field RR Lyrae (RRL) variables, based on both proprietary and publicly available spectr…

astro-ph.SR2026

High-Precision Near-Infrared Abundances of Solar Analogs in the YJ Bands

Noriyuki Matsunaga, Takuji Tsujimoto, Daisuke Taniguchi +12

We present a near-infrared abundance analysis of 46 solar analogs with known ages, observed with the WINERED WIDE-mode spectrograph at a resolution of . Using an empi…

astro-ph.SR2025

Stellar population astrophysics (SPA) with the TNG. The Phosphorus abundance on the young side of MilkyWay

Mingjie Jian, Xiaoting Fu, Valentina D'Orazi +11

We present phosphorus abundance measurements for a total of 102 giant stars, including 82 stars in 24 open clusters and 20 Cepheids, based on high-resolution near-infrared spectra…

astro-ph.SR2025

The elderly among the oldest: new evidence for extremely metal-poor RR Lyrae stars

Valentina D'Orazi, Vittorio F. Braga, Giuseppe Bono +21

We performed a detailed spectroscopic analysis of three extremely metal-poor RR Lyrae stars, exploring uncharted territories at these low metallicities for this class of stars. Usi…

astro-ph.SR2024★ 5 cited

Stellar population astrophysics (SPA) with the TNG: Measurement of the He I 10830Å line in the open cluster Stock 2

Mingjie Jian, Xiaoting Fu, Noriyuki Matsunaga +10

The precise measurement of stellar abundances plays a pivotal role in providing constraints on the chemical evolution of the Galaxy. However, before spectral lines can be employed…

astro-ph.SR2023★ 5 cited

Exploring Be phenomena in OBA stars: a Mid-infrared search

Mingjie Jian, Noriyuki Matsunaga, Biwei Jiang +2

As early-type stars with a rotation speed close to their critical velocity, Be stars experience an event called the Be phenomenon. The material in their equator is ejected into out…