139 citations · 1.8k across the 70 of their papers we have counts for
72 papers
ALMA Observations of DEM L241/LMC P3 in the Large Magellanic Cloud: Evidence for the Formation of Cool Molecular Jets Driven by a Microquasar
Yasuo Fukui, Bhuvana G. R., Hidetoshi Sano +17
We present ALMA observations of DEML 241/LMC P3, the most luminous -ray binary consisting of a compact object and an O star, in CO emission. We have found an one-sided jet-like…
SKAO and Gamma-Ray Synergies
Gianluca Castignani, Gavin Rowell, Arnau Aguasca-Cabot +26
A wide variety of Galactic and extragalactic sources are known to emitradiation across the entire electromagnetic spectrum, including both transient and steady-state phenomena. A f…
New radio continuum study of the Large Magellanic Cloud Supernova Remnant N49
M. Ghavam, M. D. Filipović, R. Z. E. Alsaberi +12
We present new Australia Telescope Compact Array (ATCA) radio observations toward N49, one of the brightest extragalactic Supernova remnants (SNRs) located in the Large Magellanic…
First Study of the Supernova Remnant Population in the Large Magellanic Cloud with eROSITA
Federico Zangrandi, Katharina Jurk, Manami Sasaki +11
The study of the entire population of SNRs in a galaxy helps us to understand the underlying stellar populations, the environments, in which the SNRs are evolving, and the stellar…
Gamma-ray detection of newly discovered Ancora SNR: G288.8-6.3
Christopher Burger-Scheidlin, Robert Brose, Jonathan Mackey +5
The supernova remnant (SNR) G288.8-6.3 was recently discovered as a faint radio shell at large Galactic latitude using observations with ASKAP in the EMU survey. Here, we make the…
Discovery of a molecular cloud possibly associated with the youngest Galactic SNR G1.9+0.3
Rei Enokiya, Hidetoshi Sano, Miroslav D. Filipovic +2
The youngest known Galactic supernova remnant (SNR) G1.9+0.3 has high-velocity supernova shock beyond 10000 km s-1, and it is considered to be one of the major candidates of a PeVa…