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Inspired by the night sky. Interested in the latest research and readings in astronomy.

The fastest spinning object ever measured is a millisecond pulsar, rotating at ~24% the speed of light.

A new study says that with SKA, we should find a handful more of these that could be spinning slightly faster. But there are unlikely any sub-millisecond pulsars.

There are numerous reasons / theories as to why there is an upper limit for pulsars spinning at higher frequencies, for example, the breakup velocity (they are very well held together!) and the spin-down induced by gravitational radiation.

This science tells us about matter under these extreme conditions!

https://arxiv.org/abs/2312.12185

#Pulsars #RadioAstronomy #Astrophysics #NuclearPhysics #Astrodon

On the spin period distribution of millisecond pulsars

Spin period distribution provides important clues to understand the formation of millisecond pulsars (MSPs). To uncover the intrinsic period distribution, we analyze three samples of radio MSPs in the Galactic field and in globular clusters. The selection bias due to pulse broadening has been corrected but turns out to be negligible. We find that all the samples can be well described by a Weibull distribution of spin frequencies. Considering MSPs in the Galactic field or in globular clusters, and in isolation or in binary systems, we find no significant difference in the spin distribution among these subpopulations. Based on the current known population of MSPs, we find that sub-millisecond pulsars are unlikely to be discovered by the Square Kilometer Array, although up to $\sim10$ discoveries of pulsars that spin faster than the current record holder of $P=1.4$~ms are expected.

arXiv.org

Mysterious New Signals Detected by SETI: Unlocking the Strange Puzzle of Fast Radio Bursts

https://scitechdaily.com/mysterious-new-signals-detected-by-seti-unlocking-the-strange-puzzle-of-fast-radio-bursts/

"A team of @setiinstitute scientists have unveiled new insights into a cosmic mystery known as Fast Radio Bursts (FRBs). The discovery and detailed observation of the repeating FRB 20220912A, made at the SETI Institute’s upgraded Allen Telescope Array (ATA), shed light on the nature of these space signals."

#SETI #Astrodon #astronomy #FRBs

Mysterious New Signals Detected by SETI: Unlocking the Strange Puzzle of Fast Radio Bursts

This work proves that new telescopes with unique capabilities, like the ATA, can provide a new angle on outstanding mysteries in FRB science. A team of SETI Institute scientists have unveiled new insights into a cosmic mystery known as Fast Radio Bursts (FRBs). The discovery and detailed observat

SciTechDaily

Why are open clusters and globular clusters found in different places?

https://www.astronomy.com/science/why-are-open-clusters-and-globular-clusters-found-in-different-places/

"Why are open star clusters in the disk of a spiral galaxy, while globulars are in the halo? Is the same true for irregular and elliptical galaxies?"

#Astrodon #astronomy

Why are open clusters and globular clusters found in different places?

These two types of clusters form in different environments and thus evolve to exhibit different properties and live in different locations.

Astronomy Magazine

JWST was built to help study the formation of the first galaxies in the Universe, and it's already made some amazing discoveries. But with the help of gravitational lenses, it might be possible for the telescope to detect the very first stars in the Universe. They're made from the primordial elements left over from the Big Bang. They could grow enormously large and hot, explode as supernovae, and seed their regions of the Universe with heavier elements.

http://arxiv.org/abs/2312.09289

The detection and characterization of highly magnified stars with JWST: Prospects of finding Population III

Gravitational lensing may render individual high-mass stars detectable out to cosmological distances, and several extremely magnified stars have in recent years been detected out to redshifts $z\approx 6$. Here, we present Muspelheim, a model for the evolving spectral energy distributions of both metal-enriched and metal-free stars at high redshifts. Using this model, we argue that lensed stars should form a highly biased sample of the intrinsic distribution of stars across the Hertzsprung-Russell diagram, and that this bias will typically tend to favour the detection of lensed stars in evolved stages characterized by low effective temperatures, even though stars only spend a minor fraction of their lifetimes in such states. We also explore the prospects of detecting individual, lensed metal-free (Population III) stars at high redshifts using the James Webb Space Telescope (JWST). We find that very massive ($\gtrsim 100\ M_\odot$) Population III stars at $z\gtrsim 6$ may potentially be detected by JWST in surveys covering large numbers of strong lensing clusters, provided that the Population III stellar initial mass function is sufficiently top-heavy, that these stars evolve to effective temperatures $\leq 15000$ K, and that the cosmic star formation rate density of Pop III stars reaches $\gtrsim 10^{-4}\ M_\odot$ cMpc$^{-3}$ yr$^{-1}$ at $z\approx$ 6-10. Various ways to distinguish metal-free lensed stars from metal-enriched ones are also discussed.

arXiv.org

Astronomers detect almost 100 new extremely metal-poor galaxies

https://phys.org/news/2023-12-astronomers-extremely-metal-poor-galaxies.html

"Extremely metal-poor galaxies (XMPGs) are the ones with metallicity below 0.1 of the solar metallicity. Given that these galaxies are chemically unevolved, they can serve as excellent laboratories for investigating the chemical evolution theories of galaxies and studying the physical processes in the early stages of their evolution."

#astronomy #Astrodon

Astronomers detect almost 100 new extremely-metal poor galaxies

By analyzing the early data from the Dark Energy Spectroscopic Instrument (DESI), an international team of astronomers has identified 95 new extremely metal-poor galaxies at a low redshift. The finding is detailed in a paper published December 1 on the pre-print server arXiv.

Phys.org
James Webb telescope discovers oldest black hole in the universe

The James Webb Space Telescope’s discovery of the universe's oldest black holes is giving astronomers some vital clues for how they came to be.

Live Science

Biggest solar flare in years temporarily disrupts radio signals on Earth

https://apnews.com/article/solar-flare-sun-nasa-eb3389b4e41955c3292b9c917a5667dc

"The sun is nearing the peak of its 11-year or so solar cycle. Maximum sunspot activity is predicted for 2025."

#astronomy #Astrodon

Biggest solar flare in years temporarily disrupts radio signals on Earth

A NASA telescope has captured the biggest solar flare in years, which temporarily knocked out radio communication on Earth. The sun spit out the huge flare along with a massive radio burst on Thursday, leading to two hours of radio interference in the U.S. and other sunlit parts of the world. The government's Space Weather Prediction Center says multiple pilots reported communication disruptions, with the impact felt across the country. Scientists are now analyzing a possible coronal mass ejection directed at Earth that could cause a geomagnetic storm. NASA's Solar Dynamics Observatory caught the action in extreme ultraviolet light.

AP News

New clues emerge toward possible life on Enceladus

https://www.astronomy.com/science/new-clues-emerge-toward-possible-life-on-enceladus/

"'Sulfur and phosphorus are two elements required for life, along with carbon, hydrogen, nitrogen, and oxygen,' Peter says. If the existence of sulfur is confirmed — phosphorus was detected at Enceladus earlier this year — this knowledge will help to empower the building of an Enceladus explorer."

#Astrodon #astronomy #Enceladus

New clues emerge toward possible life on Enceladus | Astronomy.com

Enceladus has a variety of important organic compounds that hint it may harbor an environment conducive to life deep within its oceans.

Astronomy Magazine

A Planetary System With Six Sub-Neptunes Locked in Perfect Resonance

https://www.seti.org/planetary-system-six-sub-neptunes-locked-perfect-resonance

“This discovery is going to become a benchmark system to study how sub-Neptunes, the most common type of planets outside of the solar system, form, evolve, what are they made of, and if they possess the right conditions to support the existence of liquid water in their surfaces.”

#NASA #Exoplanets #TESS #Astrodon #astronomy

A Planetary System With Six Sub-Neptunes Locked in Perfect Resonance

A team of researchers led by University of Chicago astronomer Rafael Luque analyzed data acquired by both NASA’s Transiting Exoplanet Survey Satellite (TESS) and ESA’s CHaracterising ExOPlanet Satellite (Cheops) and found a unique planetary system. Orbiting a star cataloged as HD110067, this system contains six sub-Neptune planets.

SETI Institute

Webb identifies tiniest free-floating brown dwarf

https://phys.org/news/2023-12-webb-tiniest-free-floating-brown-dwarf.html

"This is the first time we've detected this molecule in the atmosphere of an object outside our solar system [..] Models for brown dwarf atmospheres don't predict its existence. We're looking at objects with younger ages and lower masses than we ever have before, and we're seeing something new and unexpected."

#JWST #Astrodon #astronomy

Webb identifies tiniest free-floating brown dwarf

Brown dwarfs are sometimes called failed stars, since they form like stars through gravitational collapse, but never gain enough mass to ignite nuclear fusion. The smallest brown dwarfs can overlap in mass with giant planets. In a quest to find the smallest brown dwarf, astronomers using the NASA/ESA/CSA James Webb Space Telescope have found the new record-holder: an object weighing just three to four times the mass of Jupiter.

Phys.org