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Research published in Astronomy & Astrophysics has cast doubt on the supposed discovery of an intermediate-mass black hole in the star cluster Omega Centauri. Initial findings suggested a black hole with a mass equivalent to 8,200 times that of the Sun resided at the cluster’s core. However, a reanalysis indicates the high-velocity stars in this dense region could instead be influenced by a cluster of stellar-mass black holes. According to Justin Read, a physicist at the University of Surrey, in a statement, the likelihood of an intermediate black hole now appears slim, with its mass potentially less than 6,000 solar masses.

Intermediate-mass black holes, sitting between stellar-mass and supermassive black holes, are theorised to bridge the evolutionary gap between these extremes. Despite being crucial to understanding black hole growth, their existence remains elusive. Scientists initially believed the gravitational effects of an intermediate-mass black hole in Omega Centauri were responsible for accelerating stars to high speeds. As explained by Andrés Bañares Hernández from the Instituto de Astrofísica de Canarias, to publications, investigating this cluster has refined the methods used to detect such objects.

New Data from Pulsar Observations

The revised analysis incorporated pulsar data, enhancing the accuracy of gravitational field measurements within Omega Centauri. Pulsars, the rapidly spinning remnants of collapsed stars, emit beams of radiation detectable as periodic pulses. Variations in their timing provided deeper insights into the gravitational dynamics of the cluster. This data led researchers to conclude that stellar-mass black holes, rather than an intermediate-mass black hole, are the likely cause of observed stellar velocities.

Future Prospects in Black Hole Research

While the study has not confirmed the existence of an intermediate-mass black hole in Omega Centauri, the researchers remain optimistic. According to Read, in his statment, ongoing advancements in pulsar timing techniques are expected to enhance the precision of black hole searches. These findings also offer a platform for understanding pulsar formation within dense star clusters.

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FAST Telescope Detects New Pulsar PSR J1922+37 in Open Cluster NGC 6791

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FAST Telescope Detects New Pulsar PSR J1922+37 in Open Cluster NGC 6791

A new pulsar, PSR J1922+37, has been discovered with a spin period of 1.92 seconds using the Five-hundred-metre Aperture Spherical Radio Telescope (FAST) in China, according to a report. The finding was made in the direction of the open cluster NGC 6791. If confirmed as a member of this cluster, it would be the first pulsar identified in an open cluster, a breakthrough in pulsar and stellar cluster research, according to sources.

Key Details of PSR J1922+37

The finding was reported in a paper published Dec. 11 on the arXiv preprint server. As per reports, the pulsar PSR J1922+37 has been observed with a dispersion measure of 85 pc/cm³ and a flux density of approximately 7.0 µJy. Its position aligns closely with the location of NGC 6791, with an offset of 14 arcminutes from the cluster’s centre. The estimated distance of the pulsar, 15,600 light-years, is consistent with the cluster’s distance range, which is calculated to be between 13,100 and 16,000 light-years.

According to the study, led by Xiao-Jin Liu of Beijing Normal University, the dense stellar environment of NGC 6791 increases the likelihood of pulsars being present within the cluster. Researchers have suggested that precise measurements of PSR J1922+37’s distance and proper motion will be necessary to confirm its association with NGC 6791.

Potential for Further Discoveries

The researchers indicated that NGC 6791’s compact and high surface brightness environment could host additional pulsars. An estimate provided in the study predicts that as many as nine pulsars may exist within this cluster. The team noted that further observations using advanced techniques could help verify these predictions.

The report further highlights that the discovery has been described as a significant development in the understanding of pulsars within open clusters, an area of study previously limited due to low stellar density in such regions. Verification of PSR J1922+37’s cluster membership will require additional studies, including proper motion analysis to establish a definitive connection.

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Alien Plant Fossil in Utah Stumps Scientists, Defies Known Plant Families

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Alien Plant Fossil in Utah Stumps Scientists, Defies Known Plant Families

Fossilised plant remains unearthed near the now-abandoned town of Rainbow, Utah, have defied classification. The plant, named Othniophyton elongatum, was initially discovered in 1969, but recent analysis has shown it is unrelated to any known plant families, living or extinct. The fossil, dating back around 47 million years, was preserved in the Green River Formation, a region noted for its well-preserved ancient flora and fauna.

The article was published in the journal Annals of Botany. As per reports, researchers, led by Steven Manchester, curator of palaeobotany at the Florida Museum of Natural History, examined a more complete specimen discovered in the University of California, Berkeley’s palaeobotany collection. This specimen, featuring leaves, flowers and fruits, provided additional details that contradicted the earlier theory linking the plant to the ginseng family. He told Live Science that the detailed structures of the fruits and flowers show traits that have not been found in any modern or extinct plant family.

Unique Features of the Fossilised Plant

As per reports, the study revealed unique characteristics, including stamens that remained attached to the fruit even after fertilisation — a feature not observed in any other known species. Microscopy and artificial intelligence technology allowed researchers to identify micro-impressions of seeds and developing reproductive structures, adding further depth to the analysis.

Despite thorough comparisons, the researchers could not match the fossil to any of the over 400 families of flowering plants. Attempts to associate it with extinct plant groups also proved unsuccessful, as reported.

The Green River Formation’s Role in Fossil Discoveries

The Green River Formation, known for its rich deposits of lake sediment and volcanic ash, has previously yielded other enigmatic fossils, such as Bonanzacarpum fruit and Palibinia leaves. These findings have led to the identification of extinct groups, yet Othniophyton elongatum continues to challenge classification efforts. According to sources, the findings highlight the complexity of ancient ecosystems and suggest that the fossil record still holds many untold stories of plant evolution.

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Shark Gut Design Enables Valve-Free Pipes for Efficient Fluid Flow

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Shark Gut Design Enables Valve-Free Pipes for Efficient Fluid Flow

Pipes designed to enable one-way liquid flow without the use of valves have been developed, drawing inspiration from the intestinal structure of sharks. Tesearchers at the University of Washington have created tubes featuring an internal helix, which mimics the corkscrew-shaped intestines found in sharks. This design may pave the way for more durable fluid transport systems by eliminating the need for traditional valves. The intestinal structure of sharks, which naturally restricts flow to a single direction, was studied to determine its potential applications in engineering.

The team published its findings in Proceedings of the National Academy of Sciences journal. The research was led by Sarah Keller, a chemist at the University of Washington, who explored whether this biological mechanism could be replicated in synthetic systems. Keller described to Science News Explores how the investigation involved collaboration between experts in physics and materials chemistry to ensure thorough testing and development of the concept.

Rigid and Flexible Helices Tested

The research team used 3D printing to create rigid tubes that replicated the shark intestine’s helical structure. Each tube featured variations in the size, angle, and density of the coils. These designs were tested with water flow to assess their efficiency in promoting one-way movement.

According to report, tubes with a downward-facing helix were shown to allow water to flow two to three times faster compared to configurations with an upward orientation. Ido Levin, a physicist involved in the study, explained that the downward configuration mirrored the natural orientation of shark intestines, resulting in optimal flow performance.

The report further highlights that the flexible versions of the tubes were also produced to observe the effects of deformability on fluid dynamics. Levin stated that the flow speed increased significantly—up to 15 times faster—when the helix was pointed downward in the flexible tubes. Keller noted in a statement that the interaction between the tube’s material and the flowing liquid remains under investigation to fully understand this effect.

Future Applications Considered

Potential applications for this technology have been highlighted, particularly in areas where reliability is critical. Alshakim Nelson, a materials chemist on the team, indicated in a statement, that such valve-free pipes could be useful in drainage systems or air-flow mechanisms, where traditional valves may fail due to wear over time. The absence of moving parts in this design is believed to enhance durability and reduce maintenance requirements.

Experts have noted the significance of these findings for both engineering and the understanding of natural systems. The study’s results underscore how observations from nature can inspire innovative solutions to common technical challenges. Further exploration is anticipated to determine additional uses for these one-way flow systems.

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