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@arXiv_astrophGA_bot@mastoxiv.page
2026-07-21 09:21:21

Crosslisted article(s) found for astro-ph.GA. arxiv.org/list/astro-ph.GA/new
[1/2]:
- From Triadic Interactions to Kolmogorov Scaling: A Deterministic, Scale-Resolved Formulation of E...
Erik Bertram
arxiv.org/abs/2607.16381 mastoxiv.page/@arXiv_physicsfl
- Dynamical friction in stratified stellar envelopes
Damien Gagnier
arxiv.org/abs/2607.16422 mastoxiv.page/@arXiv_astrophSR
- Simultaneous radio, optical and X-ray monitoring of hard X-ray selected AGN: a variability study
L. Hern\'andez-Garc\'ia, F. Panessa, D. Williams-Baldwin, P. Ar\'evalo, A. M. Mu\~noz Arancibia
arxiv.org/abs/2607.16423 mastoxiv.page/@arXiv_astrophHE
- Origin of the Sloshing Spiral in the Abell 2107 Galaxy Cluster
Muhammed K{\i}yami Erdim
arxiv.org/abs/2607.16496 mastoxiv.page/@arXiv_astrophCO
- Determination of [Fe/H] in Fundamental mode Classical Cepheids from Gaia DR3 light curve Fourier ...
Roberto Molinaro, et al.
arxiv.org/abs/2607.16775 mastoxiv.page/@arXiv_astrophSR
- Escaped White Dwarf Candidates from Open Clusters
Huahui Yan, David R. Miller, Jingkun Zhao, Jincheng Guo, Chengyuan Li
arxiv.org/abs/2607.16815 mastoxiv.page/@arXiv_astrophSR
- Magnetic fields in Massive Star-Forming Regions (MagMaR). VIII. Magnetic field overrun by gravity...
M. Fern\'andez-L\'opez, et al.
arxiv.org/abs/2607.17160 mastoxiv.page/@arXiv_astrophSR
- Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots
Jun-Rong Liu, Hua Feng, Luis C. Ho
arxiv.org/abs/2607.17448 mastoxiv.page/@arXiv_astrophHE
- Binary White Dwarfs as Gravitational Wave Sources for LISA
Sreeta Roy, Surajit Kalita, Tomasz Bulik, Dorota Gondek-Rosi\'nska
arxiv.org/abs/2607.17787 mastoxiv.page/@arXiv_astrophSR
- Intracluster light and dark matter halo shapes reflect common assembly, not mutual coupling: shap...
Martin, Hatch, Cui, Fernandez, Bah\'e, Fischer, Montes, Pearce, Sabiu, Yepes, Yoo
arxiv.org/abs/2607.17792 mastoxiv.page/@arXiv_astrophCO
toXiv_bot_toot

@radioeinsmusicbot@mastodonapp.uk
2026-05-02 08:06:40

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