activity
20102021
most citedRed Supergiant Stars in the Large Magellanic Cloud: I. The Period-Luminosity Relation

59 citations · 210 across the 8 of their papers we have counts for

collaborators

15 papers

astro-ph.SR202116 cited

Evolved Massive Stars at Low-metallicity IV. Using 1.6 m "H-bump" to identify red supergiant stars: a case study of NGC 6822

Ming Yang, Alceste Z. Bonanos, Biwei Jiang +9

We present a case study of using a novel method to identify red supergiant (RSG) candidates in NGC 6822, based on their 1.6 m "H-bump". We collected 32 bands of photometric data…

astro-ph.SR202029 cited

Evolved Massive Stars at Low-metallicity III. A Source Catalog for the Large Magellanic Cloud

Ming Yang, Alceste Z. Bonanos, Biwei Jiang +9

We present a clean, magnitude-limited (IRAC1 or WISE115.0 mag) multiwavelength source catalog for the LMC. The catalog was built upon crossmatching () and deblending ($3…

astro-ph.SR202040 cited

"Ears" formation in Supernova Remnants: Overhearing an interaction history with bipolar circumstellar structures

A. Chiotellis, P. Boumis, Z. T. Spetsieri

A characteristic feature that is frequently met in nearby supernova remnants (SNRs) is the existence of two antisymmetric, local protrusions that are projected as two "ears" in the…

astro-ph.SR2020

First systematic high-precision survey of bright supernovae I. Methodology for identifying early bumps

E. Paraskeva, A. Z. Bonanos, A. Liakos +2

Rapid variability before and near the maximum brightness of supernovae has the potential to provide a better understanding of nearly every aspect of supernovae, from the physics of…

astro-ph.SR202027 cited

Evolved Massive Stars at Low-metallicity II. Red Supergiant Stars in the Small Magellanic Cloud

Ming Yang, Alceste Z. Bonanos, Bi-Wei Jiang +9

We present the most comprehensive RSG sample for the SMC up to now, including 1,239 RSG candidates. The initial sample is derived based on a source catalog for the SMC with conserv…

astro-ph.SR2020

The Interaction of Type Ia Supernovae with Planetary Nebulae: the Case of Kepler's Supernova Remnant

A. Chiotellis, P. Boumis, Z. T. Spetsieri

One of the key methods for determining the unknown nature of Type Ia supernovae (SNe Ia) is the search for traces of interaction between the SN ejecta and the circumstellar structu…