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20242026
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Showing astro-ph.SRShow all

5 papers · 1 filter

astro-ph.SR2025

Optical spectroscopic signatures of the red giant evolutionary state

Ella Xi Wang, Melissa Ness, Thomas Nordlander +17

Modern spectroscopic surveys output large data volumes. Theoretical models provide a means to transform the information encoded in these data to measurements of physical stellar pr…

astro-ph.SR2025

Multiple generation star formation in Cepheus Flare

Fan Wang, Min Fang, Xiaoting Fu +8

We present an analysis of the young stellar moving group ASCC 127 using Gaia DR3 data, significantly expanding its membership to 3,971 stars -- double the number identified in prev…

astro-ph.SR2025

Revisiting open clusters within 200 pc in the solar neighbourhood with Gaia DR3

Penghui Liu, Min Fang, Yue-Lin Sming Tsai +3

In this study, we develop a membership identification method and apply it for 30 open clusters (OCs) within 200 pc of the Sun using astrometric data of Gaia DR3. By accounting for…

astro-ph.SR2024

Empirical color correction to MIST and PARSEC isochrones on Gaia BR-RP and G-RP with benchmark open clusters

Fan Wang, Min Fang, Xiaoting Fu +8

Recent literature reports a color deviation between observed Gaia color-magnitude diagrams (CMDs) and theoretical model isochrone predictions, particularly in the very low-mass reg…

astro-ph.SR2024

Stellar population astrophysics (SPA) with the TNG: Measurement of the He I 10830Ã 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…