Chandra/HETG and NuSTAR Observations of V750 Ara, a $γ,$Cas-type Star

Kavli Affiliate: David P. Huenemoerder | First 5 Authors: David P. Huenemoerder, David P. Huenemoerder, , , | Summary: We present 197 ks HETG and 95 ks NuSTAR spectra of the $gamma,$Cas-type object V750 Ara. The high-resolution X-ray spectra show that the target is similar to other objects of this class. Data are interpreted under […]


Continue.. Chandra/HETG and NuSTAR Observations of V750 Ara, a $γ,$Cas-type Star

BEES: Quasar lifetime measurements from extended rest-optical emission line nebulae at $zsim6$

Kavli Affiliate: Robert A. Simcoe | First 5 Authors: Dominika Ďurovčíková, Dominika Ďurovčíková, , , | Summary: Measurements of quasar lifetimes at high redshift indicate that the earliest billion-solar-mass supermassive black holes (SMBHs) have only been active as luminous quasars for less than a million years. Recently, extended Ly$alpha$ nebulae around $zsim6$ quasars have revealed […]


Continue.. BEES: Quasar lifetime measurements from extended rest-optical emission line nebulae at $zsim6$

A Sharper View of the X-ray Spectrum of MCG–6-30-15 with XRISM, XMM-Newton and NuSTAR

Kavli Affiliate: Erin Kara | First 5 Authors: Laura W. Brenneman, Laura W. Brenneman, , , | Summary: We present a time-averaged spectral analysis of the 2024 XRISM observation of the narrow-line Seyfert-1 galaxy MCG–6-30-15, taken contemporaneously with XMM-Newton and NuSTAR. Our analysis leverages a unique combination of broadband and high-resolution X-ray spectroscopy to definitively […]


Continue.. A Sharper View of the X-ray Spectrum of MCG–6-30-15 with XRISM, XMM-Newton and NuSTAR

XRISM/Resolve observations of Hercules X-1: vertical structure and kinematics of the disk wind

Kavli Affiliate: Erin Kara | First 5 Authors: Peter Kosec, Peter Kosec, , , | Summary: X-ray binary accretion disk winds can carry away a significant fraction of the originally infalling matter and hence strongly affect the accretion flow and the long-term evolution of the binary system. However, accurate measurements of their mass outflow rates […]


Continue.. XRISM/Resolve observations of Hercules X-1: vertical structure and kinematics of the disk wind

Stacking 21-cm Maps around Lyman-$α$ Emitters during Reionization: Prospects for a Cross-correlation Detection with the Hydrogen Epoch of Reionization Array

Kavli Affiliate: Jacqueline N. Hewitt | First 5 Authors: Kai-Feng Chen, Kai-Feng Chen, , , | Summary: Observations of the redshifted 21-cm line during the Epoch of Reionization will open a new window to probe the intergalactic medium during the formation of the first stars, galaxies, and black holes. A particularly promising route to an […]


Continue.. Stacking 21-cm Maps around Lyman-$α$ Emitters during Reionization: Prospects for a Cross-correlation Detection with the Hydrogen Epoch of Reionization Array

JWST-TST High Contrast: Medium-resolution spectroscopy reveals a carbon-rich circumplanetary disk around the young accreting exoplanet Delorme 1 AB b

Kavli Affiliate: Sara Seager | First 5 Authors: Mathilde Mâlin, Mathilde Mâlin, , , | Summary: Young accreting planetary-mass objects are thought to draw material from a circumplanetary disk (CPD) composed of gas and dust. While the gas within the disk is expected to disperse within the first million years, strong accretion has nonetheless been […]


Continue.. JWST-TST High Contrast: Medium-resolution spectroscopy reveals a carbon-rich circumplanetary disk around the young accreting exoplanet Delorme 1 AB b

Comparing XRISM cluster velocity dispersions with predictions from cosmological simulations: are feedback models too ejective?

Kavli Affiliate: Erin Kara | First 5 Authors: XRISM Collaboration, XRISM Collaboration, , , | Summary: The dynamics of the intra-cluster medium (ICM), the hot plasma that fills galaxy clusters, are shaped by gravity-driven cluster mergers and feedback from supermassive black holes (SMBH) in the cluster cores. XRISM measurements of ICM velocities in several clusters […]


Continue.. Comparing XRISM cluster velocity dispersions with predictions from cosmological simulations: are feedback models too ejective?

Studying the gravitational-wave population without looking that FAR out

Kavli Affiliate: Salvatore Vitale | First 5 Authors: Noah E. Wolfe, Noah E. Wolfe, , , | Summary: From catalogs of gravitational-wave transients, the population-level properties of their sources and the formation channels of merging compact binaries can be constrained. However, astrophysical conclusions can be biased by misspecification or misestimation of the population likelihood. Despite […]


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First X-ray and radio polarimetry of the neutron star low-mass X-ray binary GX 17+2

Kavli Affiliate: Herman L. Marshall | First 5 Authors: Unnati Kashyap, Unnati Kashyap, , , | Summary: We report the first polarimetric results of the neutron star (NS) low-mass X-ray binary (LMXB) Z-source GX 17+2 using the Imaging X-ray Polarimetry Explorer (IXPE) and the Very Large Array (VLA). We find that the X-ray source was […]


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Self-interacting dark matter in the center of a Local Group dwarf galaxy and its satellites

Kavli Affiliate: Mark Vogelsberger | First 5 Authors: Thales A. Gutcke, Thales A. Gutcke, , , | Summary: We present a detailed comparison of a Local Group dwarf galaxy analogue evolved in two cosmological models: the standard $Lambda$CDM and a self-interacting dark matter (SIDM) model with a velocity-dependent cross-section. Both simulations are run with the […]


Continue.. Self-interacting dark matter in the center of a Local Group dwarf galaxy and its satellites