#metallicity

2025-11-29

Weekly Update from the Open Journal of Astrophysics – 29/11/2025

It’s Saturday again, so it’s time for the usual update of the week’s new papers at the Open Journal of Astrophysics. Publishing this week was interrupted by the Thanksgiving holiday in the United States, which meant there were no arXiv announcements yesterday. Nevertheless, since the last update we have published another four papers, which brings the number in Volume 8 (2025) up to 184, and the total so far published by OJAp up to 419.

The first paper this week is “A theoretical prediction for the dipole in nearby distances using cosmography” by Hayley J. Macpherson (U. Chicago, USA) and Asta Heinesen (Niels Bohr Institute, Denmark). This was published on Monday 24th November 2025 in the folder Cosmology and Nongalactic Astrophysics. It presents a method to predict the dipole in luminosity distances that arises due to nearby inhomogeneities to leading-order correction to the standard isotropic distance-redshift law. Incidentally, I wrote about a talk by one of the authors here.

The overlay is here:

 

You can find the officially accepted version on arXiv here and the Fediverse announcement is here:

Open Journal of Astrophysics

@OJ_Astro@fediscience.org

New Publication at the Open Journal of Astrophysics: "A theoretical prediction for the dipole in nearby distances using cosmography" by Hayley J Macpherson (U. Chicago, USA) and Asta Heinesen (Niels Bohr Institute, Denmark)

doi.org/10.33232/001c.150319

November 24, 2025, 8:25 am 2 boosts 1 favorites

 

The second paper of the week is “A Targeted Gamma-Ray Search of Five Prominent Galaxy Merger Systems with 17 years of Fermi-LAT Data” by Siddhant Manna and Shantanu Desai (IIT Hyderabad Kandi, India). This one was published on Tuesday November 25th 2025 in the folder marked High-Energy Astrophysical Phenomena. It describes a search for gamma-ray emission in Fermi-LAT data from five merging galaxy systems with marginal detections for two of them

The overlay is here:

 

You can find the official version of this one on arXiv here. The federated announcement on Mastodon is here:

 

Next one up is “Metallicity fluctuation statistics in the interstellar medium and young stars – II. Elemental cross-correlations and the structure of chemical abundance space” by Mark R. Krumholz (ANU, Australia), Yuan-Sen Ting (Ohio State U., USA), Zefeng Li (Durham U., UK), Chuhan Zhang (ANU), Jennifer Mead (Columbia U., USA) and Melissa K. Ness (ANU). This was published in the folder Astrophysics of Galaxies on Wednesday November 26th. It presents an extended stochastically-forced diffusion model for the chemical evolution of galaxies, making quantitative predictions for the degree of correlation in abundance patterns in both gas and young stars.

The overlay is here:

 

You can find the official accepted version on arXiv here. The fediverse announcement is here:

Open Journal of Astrophysics

@OJ_Astro@fediscience.org

New Publication at the Open Journal of Astrophysics: "Metallicity fluctuation statistics in the interstellar medium and young stars – II. Elemental cross-correlations and the structure of chemical abundance space" by Mark R. Krumholz (ANU, Australia), Yuan-Sen Ting (Ohio State U., USA), Zefeng Li (Durham U., UK), Chuhan Zhang (ANU), Jennifer Mead (Columbia U., USA) and Melissa K. Ness (ANU)

doi.org/10.33232/001c.150356

November 26, 2025, 8:34 am 1 boosts 1 favorites

The fourth and final paper of the week is “Simulating realistic Lyman-alpha emitting galaxies including the effect of radiative transfer” by Hasti Khoraminezhad & Shun Saito (Missouri Institute of Science & Technology, USA), Max Gronke (U. Heidelberg, Germany) and Chris Byrohl (MPA Garching, Germany). An empirical model for Lyman-alpha emitters (LAEs) which provides predictions for the halo occupation distributions and relationship between luminosity and halo mass, including the distribution of satellite LAEs. It was published on Thursday November 27th 2025 in the folder Astrophysics of Galaxies.

The overlay is here:

You can find the official published version on arXiv here. The Fediverse announcement follows:

Open Journal of Astrophysics

@OJ_Astro@fediscience.org

New Publication at the Open Journal of Astrophysics: "Simulating realistic Lyman-alpha emitting galaxies including the effect of radiative transfer" by Hasti Khoraminezhad & Shun Saito (Missouri Institute of Science & Technology, USA), Max Gronke (U. Heidelberg, Germany) and Chris Byrohl (MPA Garching, Germany)

doi.org/10.33232/001c.151254

November 27, 2025, 9:20 am 1 boosts 1 favorites

And that concludes the update for this week. I will do another next Saturday.

#arxiv250701095v3 #arxiv250714572v2 #arxiv250716707v2 #arxiv250806232v2 #astrophysicsOfGalaxies #chemicalAbundances #cosmography #cosmology #cosmologyAndNongalacticAstrophysics #diamondOpenAccess #diamondOpenAccessPublishing #fermiLat #galaxyMergers #gammaRay #highEnergyAstrophysicalPhenomena #lymanAlphaEmitters #metallicity #openAccess #openAccessPublishing #openJournalOfAstrophysics #theOpenJournalOfAstrophysics

German Virtual Observatorygavo@fediscience.org
2025-11-14

New in the #VirtualObservatory: “Open cluster parameters derived using Gaia XP” by Nizovkina M. et al.
cdsarc.cds.unistra.fr/viz-bin/
#OpenStarClusters #Metallicity #Extinction #StellarDistance

German Virtual Observatorygavo@fediscience.org
2025-10-25

New in the #VirtualObservatory: “Estimating [Fe/H] of RR Lyrae using Gaia DR3” by Monti L. et al.
cdsarc.cds.unistra.fr/viz-bin/
#VisibleAstronomy #VariableStars #Metallicity

molly at KillBaitmolly@killbait.com
2025-10-18

Astronomers Discover Star with Lowest Metallicity Ever Seen, Possibly a Descendant of the First Stars

Astronomers have discovered a red giant star, SDSS J0715-7334, at the edge of the Milky Way with the lowest concentration of heavy elements ever observed in a star. This star, about 85,000 light-years away, might be a direct descendant of the universe's first stars, formed from primordial hydrogen l... [More info]

German Virtual Observatorygavo@fediscience.org
2025-10-16
German Virtual Observatorygavo@fediscience.org
2025-09-28
German Virtual Observatorygavo@fediscience.org
2025-09-27
German Virtual Observatorygavo@fediscience.org
2025-09-27
German Virtual Observatorygavo@fediscience.org
2025-09-26
German Virtual Observatorygavo@fediscience.org
2025-09-15

New in the #VirtualObservatory: “RR Lyrae stars trace the Milky Way warp” by Cabrera-Gadea M. et al.
cdsarc.cds.unistra.fr/viz-bin/
#VariableStars #MilkyWayGalaxy #StellarDistance #Metallicity

German Virtual Observatorygavo@fediscience.org
2025-09-12

New in the #VirtualObservatory: “List of planets from HARPS/Coralie surveys” by Emsenhuber A. et al.
cdsarc.cds.unistra.fr/viz-bin/
#MultipleStars #Exoplanets #VisibleAstronomy #Metallicity

German Virtual Observatorygavo@fediscience.org
2025-08-16
German Virtual Observatorygavo@fediscience.org
2025-08-08

New in the #VirtualObservatory: “GD-1 and Kshir tidal streams metallicity and motion” by Shi W.B. et al.
cdsarc.cds.unistra.fr/viz-bin/
#MilkyWayGalaxy #GiantStars #RadialVelocity #Metallicity

ƧƿѦςɛ♏ѦਹѤʞspacemagick
2025-07-21
German Virtual Observatorygavo@fediscience.org
2025-07-05
2025-05-04

Pebble accretion is the leading theory for the formation of #exoplanets more massive than the Earth.

But any parameters influence #planet growth in the pebble accretion models, including pebble fragmentation velocity, turbulence strength, stellar #metallicity, stellar mass, and planet location.

Planets orbiting #stars with higher metallicity have an overall higher probability of reaching their pebble isolation mass than those orbiting lower metallicity stars, but the impact of metallicity is not as high as that of stellar mass, orbital separation, and most importantly disc turbulence.

#astronomy
astrobiology.com/2025/05/can-c

2025-02-06

Using the sun as a baseline, astronomers can measure when a #star formed by determining its #metallicity, or the level of heavy elements present within it.

Metal-rich #stars or nebulas formed relatively recently, while metal-poor objects were likely present during the early #universe.

The formation of super-Earths, #planets more massive than the Earth, near metal-poor stars is significantly more difficult than near high-metalliciry ones.

#exoplanets #astronomy
astrobiology.com/2024/09/forma

2024-11-17
2024-10-08

New in the #VirtualObservatory: “CaII triplet stellar-activity indices from LAMOST” by Huang X. et al.
cdsarc.cds.unistra.fr/viz-bin/
#VisibleAstronomy #InfraredAstronomy #Spectroscopy #Metallicity

2024-08-24

New in the #VirtualObservatory: “Magnetic activity of G-type stars from LAMOST & TESS” by Su T. et al.
cdsarc.cds.unistra.fr/viz-bin/
#Spectroscopy #RadialVelocity #StellarSpectralTypes #Metallicity

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