activity
19962026
most citedDeep Wide-Field Spectrophotometry of the Open Cluster M67

209 citations · 1.9k across the 55 of their papers we have counts for

collaborators

55 papers

astro-ph.SR2026

Gaia24ccy: An outburst followed the footsteps of its predecessor

Koshvendra Singh, Joe P. Ninan, Zhen Guo +25

Accretion-driven outbursts in young stellar objects remain poorly understood, largely limited by a statistically small sample of closely followed-up events. This underscores the im…

astro-ph.GA2023

Binary Star Evolution in Different Environments: Filamentary, Fractal, Halo and Tidal-tail Clusters

Xiaoying Pang, Yifan Wang, Shih-Yun Tang +7

Using membership of 85 open clusters from previous studies (Pang et al. 2021a,b, 2022b; Li et al. 2021) based on Gaia DR3 data, we identify binary candidates in the color-magnitude…

astro-ph.SR2023★ 22 cited

A novel survey for young substellar objects with the W-band filter VI: Spectroscopic census of sub-stellar members and the IMF of Orionis cluster

Belinda Damian, Jessy Jose, Beth Biller +11

Low-mass stars and sub-stellar objects are essential in tracing the initial mass function (IMF). We study the nearby young Orionis cluster (d408 pc; age1.8 Myr) usi…

astro-ph.SR2022★ 15 cited

Time-Variable Jet Ejections from RW Aur A, RY Tau and DG Tau

Michihiro Takami, Hans Moritz Guenther, P. Christian Schneider +17

We present Gemini-NIFS, VLT-SINFONI and Keck-OSIRIS observations of near-infrared [Fe II] emission associated with the well-studied jets from three active T Tauri stars; RW Aur A,…

astro-ph.GA2022★ 5 cited

Star and Cluster Formation in the Sh2-112 Filamentary Cloud Complex

Alik Panja, Yan Sun, Wen Ping Chen +1

We present the star formation activity around the emission nebula Sh2-112. At a distance of ~kpc, this \ion{H}{2} complex, itself 3~pc in radius, is illuminated by the mas…

astro-ph.GA2022★ 7 cited

Revealing the dust grain polarization properties as a function of extinction and distance towards NGC 1893

N. Bijas, Chakali Eswaraiah, Jia-Wei Wang +5

Dust polarization observations at optical wavelengths help to understand the dust grain properties and trace the plane-of-the-sky component of the magnetic field. In this study, we…