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arxiv.org
http://arxiv.org > abs > 2610.25583v1
Reading Between the Lines: How Much Information Remains After Fitting a Stellar Spectrum?
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arxiv.org
http://arxiv.org > abs > 2610.24396v1
Prospects for submillimeter VLBI of black hole photon rings with a stratospheric balloon-borne telescope
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arxiv.org
http://arxiv.org > abs > 2610.24276v1
Mass-loss Rates of 74 Bow Shock OB Stars: No Evidence for Bi-stability Behavior
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arxiv.org
http://arxiv.org > abs > 2610.23452v1
Isomer-resolved ion-molecule reaction kinetics of HCO+ and HOC+
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arxiv.org
http://arxiv.org > abs > 2610.23380v1
Three-dimensional spatial modelling of nuclear de-excitation lines
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arxiv.org
http://arxiv.org > abs > 2610.23140v1
Seeing Through the RFI Mask: DT-FISTA Inpainting of Pulsar Dynamic Spectra via Fourier Sparsity
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arxiv.org
http://arxiv.org > abs > 2610.22662v1
The transformative power of ALMA2040 for mm-VLBI
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arxiv.org
http://arxiv.org > abs > 2610.22598v1
The Magnetized Universe: From planet-forming disks to the high-redshift universe
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arxiv.org
http://arxiv.org > abs > 2610.22503v1
An ALMA view on molecular complexity: water, methanol, and methyl formate in the HD 100546 and IRS 48 disks
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arxiv.org
http://arxiv.org > abs > 2610.22488v1
Contrasting geometries of kiloparsec-scale stellar flows associated with giant Galactic cavities