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A cosmic scene with bright stars and nebulae, overlaid with the logos of the American Museum of Natural History and NASA, and text: Eric Andersson, The Star-by-Star Formation of the Smallest Galaxies.

July 7, 2025

The star-by-star formation of the smallest galaxies

Eric Andersson, American Museum of Natural History

Scatter plot showing extragalactic DM versus redshift, with data points for DSA-110 FRBs, non-DSA FRBs, and Macquart et al. (2020). Inset diagram shows baryonic matter components. Title: What is the CGM?.

July 2, 2025

Probing the CGM with FRB Dispersion and Scattering

Dylan L. Jow, KIPAC

Map view showing Lake Ontario with overlays: a large white circle labeled 鈥淣eutron Star鈥� and a smaller black circle labeled 鈥淏lack Hole.鈥� Title reads 鈥淣eutron Stars & Black Holes.鈥� There is a QR code on the lower right.

May 29, 2025

Neutron Stars & Black Holes: Astrophysical Laboratories for Nuclear Physics and Nuclear Yardsticks for Astrophysical Phenomena

Reed Essick, University of Toronto

A blurry, bright yellow and orange circular spot is centered against a dark blue and black background, resembling a glowing object in space seen through an infrared or heat-sensitive camera.

April 16, 2025

Flaring Activity of the Black Hole at the Center of the Galaxy

Farhad Yusef-Zadeh, Northwestern University

An artistic illustration of two bright, white neutron stars merging in space, emitting a burst of blue and white light and surrounded by swirling clouds and stars.

December 23, 2024

Beyond the first wave: understanding binary neutron star and black hole formation channels

Lieke Van Son, Harvard University

A swirling black hole surrounded by a bright, glowing accretion disk in deep space, with scattered stars and cosmic dust filling the dark background.

December 8, 2016

Electromagnetic and Gravitational Wave Signals from Merging Black Holes and Neutron Stars

Black hole-neutron star and neutron star-neutron star mergers are powerful emitters of gravitational waves, and can produce a wide range of bright electromagnetic transients. They also provide us with a remarkable environment to study nuclear interactions in the cold, dense core of neutron stars, and may significantly contribute to the production of many heavy elements whose origin remains unexplained.