output
20042026
most citedThe Seventh Data Release of the Sloan Digital Sky Survey

5.4k citations

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463 papers · 1 filter

astro-ph.SR2026

New constraints on the binary system HD 327083 and its gaseous and dusty environments

L. Cidale, P. Marchiano, M. Kraus +11

Binary systems with circumbinary molecular and dust rings are of great interest because they provide insights into the dynamics and evolution of stellar systems and the chemistry o…

astro-ph.SR2026

Multi epoch spectroscopic variability of the B supergiant HD75149

J. Chamoun-Contreras, C. Arcos, N. Machuca +6

Massive stars continuously enrich the surrounding interstellar medium by supplying it with stellar material driven by their powerful winds. B supergiant stars (BSGs) in particular…

astro-ph.SR2026

New self-consistent theoretical descriptions for mass-loss rates of O-type stars

F. Figueroa-Tapia, J. A. Panei, M. Curé +5

Massive O-type stars lose a significant fraction of their mass through radiation-driven winds, a process that critically shapes their evolution and feedback into the interstellar m…

astro-ph.SR2025★ 1 cited

Photometric and spectroscopic variability of the blue supergiant rho Leo

V. A. Checha, A. Aret, I. Kolka +12

Context. The post-main-sequence evolution of massive stars remains poorly understood, particularly for blue supergiants. These objects play a crucial role in the dynamical and chem…

astro-ph.SR2025★ 2 cited

Episodic accretion in high-mass star formation: An analysis of thermal instability for axially symmetric disks

Vardan Elbakyan, Dennis Wehner, Rolf Kuiper +3

High-mass young stellar objects exhibit episodic accretion bursts similar to their low-mass counterparts. Understanding these outbursts is crucial for elucidating massive star form…

astro-ph.SR2025★ 1 cited

Ancient, eclipsing, tidally-locked: A blue lurker progenitor in the population of extreme-velocity star candidates

A. Bhat, M. Dorsch, S. Geier +5

Many extreme velocity candidate stars have been found based on \textit{Gaia} astrometry, but need spectroscopic confirmation. We select late-type hypervelocity star (HVS) candidate…