XRF 241001A is a low-luminosity collapsar event with a broad-line Type Ic supernova, supporting XRFs as the faint end of the long GRB population observed on-axis by a weak jet.
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6 Pith papers cite this work. Polarity classification is still indexing.
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HATS-75 b has a sub-solar metallicity atmosphere (log[M/H] ≈ -1.74) with super-solar C/O, robust CH4/CO/CO2 absorption, and an H2O upper limit, where the spectrum is best explained by stellar contamination rather than hazes.
Fast-rotating green valley galaxies maintain higher metallicities than slow-rotating ones because slow rotators experience stronger outflows and more mergers that deplete their chemical content.
CRIRES+ data detect H2O and CO in HIP 67522 b, imply a mass of 29.8 Earth masses inconsistent with JWST at 3 sigma, and show a tentative 2 sigma HDO signal with extreme deuterium enrichment.
The ROXs 12 system shows 12CO/13CO ratios of 77 and 55 in the star and companion, with a C/O ratio of 0.54 in the companion.
654 WD-FGK binaries cataloged with mostly low-mass hot white dwarfs formed via binary interactions.
citing papers explorer
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XRF 241001A/SN 2024aiiq: A Faint Soft X-ray Transient Detected by SVOM with a Broad-Line Type Ic Supernova Revealed by JWST
XRF 241001A is a low-luminosity collapsar event with a broad-line Type Ic supernova, supporting XRFs as the faint end of the long GRB population observed on-axis by a weak jet.
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GEMS JWST: HATS-75 b -- A giant planet with a sub-solar metallicity atmosphere orbiting an M-dwarf
HATS-75 b has a sub-solar metallicity atmosphere (log[M/H] ≈ -1.74) with super-solar C/O, robust CH4/CO/CO2 absorption, and an H2O upper limit, where the spectrum is best explained by stellar contamination rather than hazes.
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Contrasting evolutionary pathways of fast- and slow-rotating galaxies in the green valley
Fast-rotating green valley galaxies maintain higher metallicities than slow-rotating ones because slow rotators experience stronger outflows and more mergers that deplete their chemical content.
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Atmospheric characterization of HIP 67522 b with VLT/CRIRES+. VLT/CRIRES+ suggests a heavier planet and hints at deuterium fractionation
CRIRES+ data detect H2O and CO in HIP 67522 b, imply a mass of 29.8 Earth masses inconsistent with JWST at 3 sigma, and show a tentative 2 sigma HDO signal with extreme deuterium enrichment.
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The ESO SupJup Survey. X. A carbon isotope contrast in the young ROXs 12 system
The ROXs 12 system shows 12CO/13CO ratios of 77 and 55 in the star and companion, with a C/O ratio of 0.54 in the companion.
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Discovery and Characterization of White Dwarf-FGK Main-Sequence Binaries within the Optical Main-Sequence Locus
654 WD-FGK binaries cataloged with mostly low-mass hot white dwarfs formed via binary interactions.