795 citations
- California Institute of TechnologyUS6 papers
- Harvard UniversityUS6 papers
- Berkeley CollegeUS4 papers
- Michigan Science CenterUS4 papers
- National Institute for AstrophysicsIT4 papers
- University of California, BerkeleyUS4 papers
- Cardiff UniversityGB3 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR3 papers
- Moscow Institute of Thermal TechnologyRU3 papers
- Brera Astronomical ObservatoryIT2 papers
- CEA Paris-SaclayFR2 papers
- Center for Astrophysics Harvard & SmithsonianUS2 papers
36 papers
General Relativistic Shock Wave Solutions with Black Hole Formation: The Singular Isothermal Sphere Case
Chien-Ting J. Chen, Michael J. Cai, Fabio Pacucci
The rapid emergence at of ubiquitous populations of supermassive black holes (SMBHs) revealed by JWST and of quasars with estimated masses $M_\bullet > 10^{10} M_\odot…
JWST/NIRCam imaging of the Bipolar Planetary Nebula NGC 6537: the (Infra)red Spider, Revealed
Joel Kastner, Paula Moraga Baez, Bruce Balick +5
We present James Webb Space Telescope (JWST) near-infrared (NIRCam) Br, H, [Fe II], and PAH imaging of the molecule-rich, high-excitation bipolar planetary nebula (PN) NGC 6…
Galaxies in the Epoch of Reionization Are All Bark and No Bite -- Plenty of Ionizing Photons, Low Escape Fractions
Casey Papovich, Justin W. Cole, Weida Hu +27
Early results from JWST suggest that epoch-of-reionization (EoR) galaxies produce copious ionizing photons, which, if they escape efficiently, could cause reionization to occur too…
Development of the 220/270 GHz Receiver of BICEP Array
Keck Collaboration, Y. Nakato, P. A. R. Ade +82
Measurements of B-mode polarization in the CMB sourced from primordial gravitational waves would provide information on the energy scale of inflation and its potential form. To ach…
New Compact Object Binary Populations with Precision Astrometry (Roman White Paper)
P. Gandhi, C. Dashwood Brown, Y. Zhao +6
Compact object binaries (a black hole or a neutron star orbiting a non-degenerate stellar companion) are key to our understanding of late massive star evolution, in addition to bei…
Colour evolution of Betelgeuse and Antares over two millennia, derived from historical records, as a new constraint on mass and age
Ralph Neuhäuser, Guillermo Torres, Markus Mugrauer +4
After core hydrogen burning, massive stars evolve from blue-white dwarfs to red supergiants by expanding, brightening, and cooling within few millennia. We discuss a previously neg…