Search

An extreme flare has been seen from a supermassive black hole at redshift z = 2.6. First detected in 2018, it is 30 times brighter than similar events. The most likely cause is the shredding of a star of 30 solar masses or more.

Aarrestad et al. show that, in contrast to psychedelics, the nonhallucinogenic psychoplastogen tabernanthalog promotes neuroplasticity through 5-HT_2AR activation without immediately increasing extracellular glutamate levels or immediate early gene expression.

The combination of JWST and ALMA data here unravel the history of the gas content of a quiescent galaxy, which became quenched through an act of self-sabotage. Black-hole accretion feedback heated the galaxy’s surrounding material, preventing its accretion.

A very uncommon detached binary system with a 20.5-min orbital period has been discovered to harbour a carbon–oxygen white dwarf star and a low-mass subdwarf B star with a seven-Earth radius that traces the theoretical limit of binary evolution predicted 20 years ago.

The accretion geometry of X-ray binary Cygnus X-3 is determined here from IXPE observations. X-ray polarization reveals a narrow funnel with reflecting walls, which focuses emission, making Cyg X-3 appear as an ultraluminous X-ray source.

The discovery of a distant blazar J0410−0139 at z = 7 suggests that many similar sources existed in the early Universe, supporting the hypothesis that the rapid growth of black holes is driven by jet-enhanced or obscured accretion.

Using the GRAVITY+ instrument, dynamical measurement of the black hole mass in a quasar at a redshift of 2.3 (11 billion years ago) shows how the relationship between galaxies and black holes evolves with time.

A study reporting optical and near-infrared observations of quasars at redshifts 5.8–6.6 shows that about half have strong winds, up to 17% the speed of light, suppressing black-hole growth.

Dust-emission observations of the young (<500,000 years old) protostar IRS 63 show evidence of rings and gaps in its disk, a prerequisite of planet formation.

The SPECULOOS project detected an Earth-sized planet in a short orbit around a nearby Jupiter-sized star. This planet, SPECULOOS-3 b, is one of the most promising rocky exoplanets for detailed emission spectroscopy characterization with JWST.

Saturn-mass exoplanet HD 149026b has an atmospheric metallicity 59–276 times solar, which is greater than Saturn’s atmospheric metallicity of roughly 7.5 times solar and more correlated with bulk metallicity than planet mass.

Observations of a luminous quasar from the high-resolution spectrometer Resolve aboard XRISM revealed highly inhomogeneous wind structure outflowing from a supermassive black hole, which probably consists of up to a million clumps.

The advantage of living in cities compared with rural areas with respect to height and BMI in children and adolescents has generally become smaller globally from 1990 to 2020, except in sub-Saharan Africa.

Modeling macroscopic brain dynamics is essential but limited by the slow and intensive process of fitting models to empirical data. Here, authors introduce a dynamics-aware quantization framework and hierarchical parallelism mapping strategies to enable accurate low-precision simulations on brain-inspired chips and GPUs.

A bright, long-duration gamma-ray burst observed by the Swift observatory has hybrid high-energy properties, suggesting that its origin is the merger of a compact binary.

Galaxy GSN 069 has unprecedented eruptions of X-ray light every nine hours, which indicate fast transitions between cold and warm states and may shed light on black hole accretion.

Natural forest regeneration is key to biodiversity conservation and climate change mitigation. Here the authors present a high-resolution time-series map of the age of regenerating tropical moist forests and find that most are ≤5 years old, with forest characteristics and geography explaining patterns better than climate or human pressure.

Bacterial symbionts, such as Wolbachia species, can manipulate the sexual development and reproduction of their insect hosts. Here, the authors identify a Wolbachia protein that interacts with a host masculinization factor and leads to male killing in lepidopteran insects.

During the Cambrian Radiation, oxygenation occurred in a series of short pulses. Here, the authors quantify episodic changes in reef size, extent of habitat and in metacommunity ecological complexity associated with these oxygenation pulses by examining archaeocyath sponges.

Observations of a 3-million-year-old pre-main-sequence star with a misaligned disk reveal a giant orbiting planet; the system is ideal for studying the early formation and migration of planets.

Observations of TOI-849b reveal a radius smaller than Neptune’s but a large mass of about 40 Earth masses, indicating that the planet is the remnant core of a gas giant.

Lyman-alpha emission is one of the observational probes for the high-redshift universe. Here, the authors show several Lyman-alpha emitting companion galaxies around the hot dust-obscured galaxy W0410-091 suggesting that the galaxy evolves in a very dense environment.

An unusual ultraviolet compact object associated with a dusty starburst has been observed at a redshift of about 7.2, with a luminosity that falls between that of quasars and galaxies, possibly in transition between the two. 

Ground-based and satellite observations show that the black hole in the ultraluminous X-ray source P13 has a mass of less than 15 times that of the Sun and displays the properties that typically distinguish ultraluminous X-ray sources from other stellar-mass black holes.

Spatially resolved JWST spectroscopy of a massive, quiescent galaxy at a redshift of ~4 reveals that it formed its stars and quenched rapidly, despite being surrounded by an abundant gas reservoir and gravitationally bound to a star-bursting companion.

The high-redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy, which both imply a super-Chandrasekhar mass progenitor.

The infrared view of JWST has opened up the early Universe to study. This Perspective summarizes the key developments in our understanding of the high-redshift Universe from the first 18 months of JWST observations.

Investigations in wild bats and non-human primates in Brazil and Costa Rica inform about diverse Morbillivirus ecology in neotropical bats and host jumps, and about zoonotic potential of morbilliviruses in Latin America.

Massive galaxies in the early Universe have been shown to be forming stars at high rates. Probing the properties of individual star-forming regions is beyond the resolution and sensitivity of existing telescopes. Here, however, observations are reported of the galaxy SMMJ2135–0102 at redshift z=2.3259, which has been gravitationally magnified by a factor of 32 by a galaxy cluster lens in the foreground. The physics underlying star formation here is similar to that in local galaxies, but the energetics are very different.

By analysing plant and nematode DNA from sites all around the Arctic, it is shown that vegetation before about 10,000 years ago contained more forbs (non-graminoid herbaceous vascular plants) than previously believed, which changes our understanding about the functioning of the diverse northern ecosystem that existed at this time.

Brassica oleracea is plant species comprising economically important vegetable crops. Here, the authors report the draft genome sequence of B. oleracea and, through a comparative analysis with the closely related B. rapa, reveal insights into Brassicaevolution and divergence of interspecific genomes and intraspecific subgenomes.

Analysis of the cool brown dwarf Gliese 229 B suggests that it is actually a close binary of two less massive brown dwarfs, explaining its low luminosity and settling the conflict between theoretical predictions and measurements.

The surface of hot neutron stars is known to be covered by a thin atmosphere but observations have been unable to confirm the atmospheric composition of isolated neutron stars. An analysis of archival observations of the compact X-ray source in the centre of the Cassiopeia A supernova remnant now reveals that an extremely young carbon-atmosphere neutron star (with low magnetic field) produces a good fit to the spectrum.

A giant planet candidate roughly the size of Jupiter but more than 14 times as massive is observed by TESS and other instruments to be transiting the white dwarf star WD 1856+534.