X-ray reverberation lags are used to measure the mass of the stellar-mass black hole Cygnus X-1 for the first time.
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9 Pith papers cite this work. Polarity classification is still indexing.
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3D simulations recover the critical obliquity for disc breaking predicted by semi-analytic models and reveal additional stabilization by spiral arms that can prevent breaking.
MESA grid models find HD 20794 is a 0.80 solar-mass star aged ~9 Gyr whose observed abundances match core-collapse supernova enrichment and are preserved over Gyr timescales.
New ALMA [C II] and FIR data on PSO J083+11 at z=6.34 reveal ordered rotation, typical star-forming ratios, and no outflow signatures in either galaxy, interpreted as a pre-AGN-feedback accretion phase.
Supernova remnants destroy interstellar dust less efficiently per event in dense high-star-formation regions than in the Milky Way's diffuse medium, with destruction maximized when thermal sputtering time matches the remnant age and scaling linearly with metallicity.
Galaxies in the Shapley Supercluster core have depleted HI gas fractions and longer depletion timescales than field galaxies, consistent with starvation-driven quenching.
A robust statistical test for galaxy catalog magnitude completeness improves H0 constraints by 1.3-8.6% in GWTC-1 analyses but shows no benefit for GWTC-3 due to limited K-band coverage in GLADE+.
Identifies eight Fermi-GBM sGRBs similar to 170817A via hardness-ratio K-means clustering and estimates ~5 GW+sGRB events by end of O4.
42 supernova remnants confirmed in NGC3344 via [S II]/Hα selection, Sabbadin plots, BPT diagrams and shock models from SITELLE data.
citing papers explorer
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An X-ray reverberation mass measurement of Cygnus X-1
X-ray reverberation lags are used to measure the mass of the stellar-mass black hole Cygnus X-1 for the first time.
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The Bardeen-Petterson effect in accreting supermassive black-hole binaries: disc breaking and critical obliquity
3D simulations recover the critical obliquity for disc breaking predicted by semi-analytic models and reveal additional stabilization by spiral arms that can prevent breaking.
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A Theoretical Study of the Structure and Elemental Abundances of HD 20794
MESA grid models find HD 20794 is a 0.80 solar-mass star aged ~9 Gyr whose observed abundances match core-collapse supernova enrichment and are preserved over Gyr timescales.
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A Quasar--Companion System Without AGN Outflow at $z \sim 6$: The Case of PSO J083+11
New ALMA [C II] and FIR data on PSO J083+11 at z=6.34 reveal ordered rotation, typical star-forming ratios, and no outflow signatures in either galaxy, interpreted as a pre-AGN-feedback accretion phase.
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Destruction of the interstellar dust by a supernova
Supernova remnants destroy interstellar dust less efficiently per event in dense high-star-formation regions than in the Milky Way's diffuse medium, with destruction maximized when thermal sputtering time matches the remnant age and scaling linearly with metallicity.
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Neutral Hydrogen in the Shapley Supercluster Core I: Environmental Effects on Gas Content and Galaxy Evolution
Galaxies in the Shapley Supercluster core have depleted HI gas fractions and longer depletion timescales than field galaxies, consistent with starvation-driven quenching.
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Implementing a Robust Test of Galaxy Catalogue Completeness for Dark Siren Measurements of the Hubble Constant
A robust statistical test for galaxy catalog magnitude completeness improves H0 constraints by 1.3-8.6% in GWTC-1 analyses but shows no benefit for GWTC-3 due to limited K-band coverage in GLADE+.
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Similar Fermi-GBM sGRBs to GW/sGRB 170817A in MeV-GeV energies
Identifies eight Fermi-GBM sGRBs similar to 170817A via hardness-ratio K-means clustering and estimates ~5 GW+sGRB events by end of O4.
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3D Optical Spectroscopic Study of NGC3344 with SITELLE: I. Identification and Confirmation of Supernova Remnants
42 supernova remnants confirmed in NGC3344 via [S II]/Hα selection, Sabbadin plots, BPT diagrams and shock models from SITELLE data.