activity
19972024
most citedHydra II: a faint and compact Milky Way dwarf galaxy found in the Survey of the Magellanic Stellar History

155 citations · 461 across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.GA2024

Stellar Population near NGC 2021: Procession of Star Formation in the South Rim of Supergiant Shell LMC 4

Po-Sheng Ou, Rui-Ching Chao, You-Hua Chu +2

Supergiant shells (SGSs) are the largest interstellar structures where heated and enriched gas flows into the host galaxy's halo. The SGSs in the Large Magellanic Cloud (LMC) are s…

astro-ph.SR2023★ 1 cited

Synthetic X-ray emission from white dwarf accreting planetary material

S. Estrada-Dorado, V. Lora, J. A. Toalá +4

The emission of hard X-rays associated with white dwarfs (WD) can be generated by the presence of a stellar companion either by the companion's coronal emission or by an accretion…

astro-ph.GA2023

New Insights on 30 Dor B Revealed by High-Quality Multi-wavelength Observations

Wei-An Chen, Chuan-Jui Li, You-Hua Chu +4

The supernova remnant (SNR) 30 Dor B is associated with the \ion{H}{2} region ionized by the OB association LH99. The complex interstellar environment has made it difficult to stud…

astro-ph.SR2020★ 9 cited

Chandra observations of the planetary nebula IC 4593

J. A. Toalá, M. A. Guerrero, L. Bianchi +2

The ACIS-S camera on board the Chandra X-ray Observatory has been used to discover a hot bubble in the planetary nebula (PN) IC4593, the most distant PN detected by Chandra so far.…

astro-ph.SR2020★ 11 cited

The Bubble Nebula NGC 7635 -- testing the wind-blown bubble theory

J. A. Toalá, M. A. Guerrero, H. Todt +5

We present a multiwavelength study of the iconic Bubble Nebula (NGC 7635) and its ionising star BD602522. We obtained XMM-Newton EPIC X-ray observations to search for…

astro-ph.HE2018★ 17 cited

On the apparent absence of WR+NS systems: the curious case of WR124

J. A. Toala, L. M. Oskinova, W. -R. Hamann +8

Among different types of massive stars in advanced evolutionary stages is the enigmatic WN8h type. There are only a few Wolf-Rayet (WR) stars with this spectral type in our Galaxy.…