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Quasi Star

All articles tagged with #quasi star

Webb’s Tiny Red Dots Spark Debate Over Black Hole Birth
astronomy25 days ago

Webb’s Tiny Red Dots Spark Debate Over Black Hole Birth

NASA’s Webb has detected widespread “little red dots” whose nature is disputed: they may be distant galaxies, feeding black holes, or a new class called black hole stars powered by hidden cores. New spectra introducing Balmer breaks and revised line shapes have fueled a black hole-star/quasi-star interpretation, while others argue for traditional black holes plus dust or orientation effects. The debate is fueling tests and models about how supermassive black holes might form in the early universe, with researchers seeking distinguishing patterns and mass inferences to settle the dispute.

James Webb Spots a New Cosmic Class: a Black Hole Star Wrapped in Gas
science1 month ago

James Webb Spots a New Cosmic Class: a Black Hole Star Wrapped in Gas

Using the James Webb Space Telescope, researchers identified MoM-BH*-1—a black hole at its core surrounded by a dense gas shell that makes it look star-like, with about 100,000 solar masses and emitting energy about 100 billion times that of a typical star; it formed within 700 million years after the Big Bang. This discovery suggests many of the faint red dots seen in the early universe could be black hole stars embedded in young galaxies, potentially reshaping ideas about early black holes and galaxy growth.

Tiny Red Dots in the Early Universe Spur a New Quasi-Star Theory
science2 months ago

Tiny Red Dots in the Early Universe Spur a New Quasi-Star Theory

The James Webb Space Telescope spotted a population of compact red sources in the early universe. A quasi-star model—an unusually light black hole (~100,000 solar masses) embedded in a dense gas envelope—reproduces many observed features of these little red dots, including their brightness in visible/IR and hydrogen emission, suggesting rapid black hole growth within protogalaxies. The model, however, struggles to predict ultraviolet brightness and certain spectral/dust signatures, leaving questions for future observations.