:: Library Catalog

Imagen de Portada

Guardado en:

Detalles Bibliográficos
Autores principales:	Macrie, Colin W., Sandoval, Liliana Rivera, Cavecchi, Yuri, Wong, Tin Long Sunny, Marcano, Manuel Pichardo
Formato:	Preprint
Publicado:	2024
Materias:	Solar and Stellar Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena
Acceso en línea:	https://arxiv.org/abs/2412.05442
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

A 682-second X-ray Periodicity in CH Cygni: Evidence for a Magnetic White Dwarf
por: Marcano, Manuel Pichardo, et al.
Publicado: (2026)

Shocking and Mass Loss of Compact Donor Stars in Type Ia Supernovae
por: Wong, Tin Long Sunny, et al.
Publicado: (2024)

A Catalogue of Orbital Periods of Cataclysmic Variables and Candidates from TESS Observations
por: Dağ, Meryem K., et al.
Publicado: (2026)

Accretion from a Shock-Inflated Companion: Spinning Down Neutron Stars to Hour-Long Periods
por: Cary, Savannah, et al.
Publicado: (2025)

Mass Loss and Subsequent Thermal Evolution of Surviving Helium White Dwarfs Shocked by Thermonuclear Supernovae
por: Wong, Tin Long Sunny, et al.
Publicado: (2025)

No Period Change in Two Long-Period AM CVn Binaries
por: Green, Matthew J., et al.
Publicado: (2026)

Thermal Evolution of the Central Star in Pa 30
por: Piro, Anthony L., et al.
Publicado: (2026)

A Catalogue of Ultracompact Mass-Transferring White Dwarf Binaries
por: Green, Matthew J., et al.
Publicado: (2025)

KL Dra as a Benchmark Laboratory for Accretion-Disk Physics: Constraints from TESS and Ground-Based Surveys
por: Manzano, Luis E. Salazar, et al.
Publicado: (2026)

A second candidate magnetic helium core white dwarf and 3 other variable white dwarfs in the globular cluster NGC 6397
por: Marcano, Manuel Pichardo, et al.
Publicado: (2024)

A study of transients from ground-based surveys reveals new ultra-compact accreting white dwarf binaries
por: Kára, Jan, et al.
Publicado: (2025)

Carbon burning cannot explain puffy hypervelocity white dwarfs
por: Yamaguchi, Natsuko, et al.
Publicado: (2025)

Mass-loss, composition and observational signatures of stellar winds from X-ray bursts
por: Herrera, Yago, et al.
Publicado: (2024)

A Refined Orbital Ephemeris for the Intermediate Polar FO Aquarii and Evidence for a Period Derivative
por: Garnavich, Peter, et al.
Publicado: (2025)

Reevaluating the Origin of Detectable Cataclysmic Variables in Globular Clusters: Testing the Importance of Dynamics
por: Sandoval, Liliana Rivera, et al.
Publicado: (2024)

Formation of a Possible Black-hole Ultracompact X-ray Binary with the Shortest Orbital Period
por: Yang, Xing-Peng, et al.
Publicado: (2025)

Orbital Period Variation Analysis of the HS 0705+6700 Post-Common Envelope Binary
por: Er, Huseyin, et al.
Publicado: (2024)

The impact of metallicity on the period-luminosity relation of Mira variables
por: Fadeyev, Yuri
Publicado: (2025)

Period-luminosity and period-luminosity-metallicity relation for $δ$ Scuti Stars
por: Liu, Yan-qi, et al.
Publicado: (2025)

Type II Cepheids: Period-Luminosity-Metallicity relations for the Population II distance scale
por: Das, Susmita, et al.
Publicado: (2025)

OGLE-IV Period-Luminosity relation of the LMC: an analysis using mean and median magnitudes
por: Muñoz, Jaime, et al.
Publicado: (2024)

Period-luminosity and period-luminosity-metallicity relations for Galactic RR Lyrae stars in the Sloan bands
por: Narloch, W., et al.
Publicado: (2024)

Post-Supernova Accretion of Light Elements onto a New-Born Neutron Star and NS 1987A
por: Baz-Pérez, Natalia de Jesús, et al.
Publicado: (2025)

Stellar Parameters and Orbital Period Estimates for Composite-Spectrum sdB+MS Binaries from LAMOST
por: Li, Jiangdan, et al.
Publicado: (2026)

The Anomalous Acceleration of PSR J2043+1711: Long-Period Orbital Companion or Stellar Flyby?
por: Donlon II, Thomas, et al.
Publicado: (2024)

The VMC Survey -- LIV. Anomalous Cepheids in the Magellanic Clouds Period-Luminosity relations in the near-infrared bands
por: Sicignano, Teresa, et al.
Publicado: (2025)

Outbursts in ultra-compact AM CVn binaries
por: Ramsay, Gavin
Publicado: (2025)

Orbital Period Changes in Recurrent Nova T Corona Borealis Prove That It Is Not a Type Ia Supernovae Progenitor
por: Schaefer, Bradley E.
Publicado: (2025)

Chemical Abundances Shape History (CASH). I. A Link between Giant Planets Orbital Periods and Host Stellar C/O Ratios
por: Zhang, Ruisheng, et al.
Publicado: (2026)

Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods
por: Wanderley, Fábio, et al.
Publicado: (2025)

Unveiling Long-Period Variables in M33's Central Region: Insights into Stellar Evolution and Star Formation via Near-Infrared Photometry
por: Alizadeh, Mina, et al.
Publicado: (2025)

The Dynamics of Infall and Accretion Shocks in the Outer Disk
por: Terebey, Susan, et al.
Publicado: (2025)

Properties of Galactic Outflows Driven by Starburst at Cosmic Noon: Insights from Hydrodynamical Simulations
por: Chen, Huan, et al.
Publicado: (2026)

Orbital and Physical Properties of the Pleiades Binary 27 Tau (Atlas)
por: Torres, G., et al.
Publicado: (2025)

Follow-up on three poorly studied AM CVn stars
por: Aungwerojwit, Amornrat, et al.
Publicado: (2025)

Wind Accretion in Massive Binaries Experiencing High Mass Loss Rates: I. Dependency on Mass Ratio and Orbital Period
por: Mukhija, Bhawna, et al.
Publicado: (2025)

Spectroscopic Searches for Evolutionary Orbital Period Changes in WR+OB Binaries: the Case of WR 127 (Hen 3-1772)
por: Shaposhnikov, I. A., et al.
Publicado: (2024)

Cepheid Metallicity in the Leavitt Law (C-MetaLL) survey: IX. Metallicity dependence of Period-Wesenheit relations based on a homogeneous spectroscopic sample
por: Ripepi, V., et al.
Publicado: (2025)

Orbital statistics of multiple systems formed from small-$N$ subclusters
por: Ambrose, Hannah, et al.
Publicado: (2025)

Stellar spin in young star clusters: comparison between simulations and observations
por: Cordoni, Giacomo, et al.
Publicado: (2025)