activity
20102024
most citedA pulsar in a binary with a compact object in the mass gap between neutron stars and black holes

93 citations · 416 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE202493 cited

A pulsar in a binary with a compact object in the mass gap between neutron stars and black holes

Ewan D. Barr, Arunima Dutta, Paulo C. C. Freire +22

Among the compact objects observed in gravitational wave merger events a few have masses in the gap between the most massive neutron stars (NSs) and least massive black holes (BHs)…

astro-ph.GA202322 cited

JWST uncovers helium and water abundance variations in the bulge globular cluster NGC 6440

Mario Cadelano, Cristina Pallanca, Emanuele Dalessandro +9

We used ultra-deep observations obtained with the NIRCam aboard the James Webb Space Telescope to explore the stellar population of NGC 6440: a typical massive, obscured and contam…

astro-ph.GA20239 cited

Sulfur isotope ratios in the Large Magellanic Cloud

Y. Gong, C. Henkel, K. M. Menten +11

Sulfur isotope ratios have emerged as a promising tool for tracing stellar nucleosynthesis, quantifying stellar populations, and investigating the chemical evolution of galaxies. W…

astro-ph.GA2023

The Detection of Higher-Order Millimeter Hydrogen Recombination Lines in the Large Magellanic Cloud

Marta Sewiło, Kazuki Tokuda, Stan E. Kurtz +10

We report the first extragalactic detection of the higher-order millimeter hydrogen recombination lines (). The -, -, and -transitions have been detected toward the…

astro-ph.GA201734 cited

Kinetic temperature of massive star forming molecular clumps measured with formaldehyde. II. The Large Magellanic Cloud

X. D. Tang, C. Henkel, C. -H. R. Chen +8

The Large Magellanic Cloud (LMC), the closest star forming galaxy with low metallicity, provides an ideal laboratory to study star formation in such an environment. The classical d…

astro-ph.GA201651 cited

Stellar clusterings around "Isolated" Massive YSOs in the LMC

Ian W. Stephens, Dimitrios Gouliermis, Leslie W. Looney +10

Observations suggest that there is a significant fraction of O-stars in the field of the Milky Way that appear to have formed in isolation or in low mass clusters (100