Image de couverture de livre

Association between Recurrent Novae and Nova Super-Remnants

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteur principal:	Healy-Kalesh, Michael William
Format:	Preprint
Publié:	2024
Sujets:	Astrophysics of Galaxies High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

The Newly Discovered Nova Super-Remnant Surrounding Recurrent Nova T Coronae Borealis: Will it Light Up During the Coming Eruption?
par: Shara, Michael M., et autres
Publié: (2024)

A 70 pc-Diameter Nova Super-remnant Surrounding the Recurrent Nova RS Ophiuchi
par: Shara, Michael M., et autres
Publié: (2025)

A morphological catalogue of Nova Remnants
par: Santamaria, Edgar, et autres
Publié: (2025)

Hydrodynamic Evolution and Detectability of Nova Remnants in the Galactic Center
par: Su, Zhao, et autres
Publié: (2025)

Discovery of Two New Eruptions of the Ultrashort Recurrence Time Nova M31N 2017-01e
par: Shafter, Allen W., et autres
Publié: (2024)

Revisiting the Classics: On the Statistics of Dust Formation in Novae
par: Chong, Atticus, et autres
Publié: (2025)

The Optical Evolution of the Tycho Supernova Remnant over Three Decades
par: Winkler, P. Frank, et autres
Publié: (2025)

A 9-Month Hubble Space Telescope Near-UV Survey of M87. II. A Strongly Enhanced Nova Rate near the Jet of M87
par: Lessing, Alec M., et autres
Publié: (2023)

Discovery and Detailed Study of the M31 Classical Nova AT 2023tkw: Evidence for Internal Shocks
par: Basu, Judhajeet, et autres
Publié: (2024)

Laboratory Modeling of Supernova Remnants Collisions: Implications for Triggered Star Formation
par: Fontaine, Marin, et autres
Publié: (2025)

Shockingly Bright Warm Carbon Monoxide Molecular Features in the Supernova Remnant Cassiopeia A Revealed by JWST
par: Rho, J., et autres
Publié: (2024)

A Classification Scheme for X-ray Bright Type Ia Supernova Remnants Based on Their Circumstellar Interaction
par: Court, Travis, et autres
Publié: (2025)

The Highly Variable Wind from WD J005311, the Stellar Remnant of the Peculiar Galactic Supernova of 1181
par: Thomas, C. Alexander, et autres
Publié: (2026)

MUSE Observations Reveal Optical Coronal Iron Lines from Shock Emission in Supernova Remnant 0540-69.3
par: Tenhu, L., et autres
Publié: (2025)

The Accelerating Decline of the Mass Transfer Rate in the Recurrent Nova T Pyxidis
par: Godon, P., et autres
Publié: (2024)

A Comparative Study of the Supernova Remnant Cassiopeia A from 2013--2020 Deep [Fe II]+[Si I] Images
par: Jung, Seung-Hoon, et autres
Publié: (2026)

Galactic Super-Accreting X-ray Binaries as Super-PeVatron Accelerators
par: Wang, Jieshuang, et autres
Publié: (2025)

The Cocoon from a Massive Star's Death: VLA Radio Polarization Study of Possible Historical Supernova Remnant G7.7$-$3.7
par: Luo, Tian-Xian, et autres
Publié: (2026)

Revisiting the accretion disc spectra of Dwarf Novae and Novalike variables: implications for the standard disc model
par: Zsidi, Gabriella, et autres
Publié: (2024)

Super-Eddington Chimneys: On the Cooling Evolution of Tidal Disruption Event Envelopes
par: Tuna, Semih, et autres
Publié: (2025)

Super-Keplerian Equatorial Outflows in SS 433. Centrifugal Ejection of the Circumbinary Disk
par: Waisberg, Idel, et autres
Publié: (2018)

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

Hydrodynamic Predictions for the Next Outburst of T Coronae Borealis: It will be the Brightest Classical or Recurrent Nova Ever Observed in X-rays
par: Starrfield, S., et autres
Publié: (2025)

Is the Symbiotic Recurrent Nova T CrB Late? Recent Photometric Evolution and Comparison with Past Pre-Outburst Behaviour
par: Merc, Jaroslav, et autres
Publié: (2025)

X-Ray Flashes on Helium Novae
par: Kato, Mariko, et autres
Publié: (2024)

The Rise of Nova V1674 Herculis
par: Quimby, Robert M., et autres
Publié: (2024)

Magnetic Field Amplification during Stellar Collisions between Low-Mass Stars
par: Ryu, Taeho, et autres
Publié: (2024)

Light curves and spectra for stellar collisions between main-sequence stars in galactic nuclei
par: Ryu, Taeho, et autres
Publié: (2025)

Multidimensional Nova Simulations with an Extended Buffer and Lower Initial Mixing Temperatures
par: Clark, Alexander Smith, et autres
Publié: (2025)

A star-by-star correspondence between X-ray activity and rotation in the young open cluster NGC 2516 with eROSITA
par: Fritzewski, Dario J., et autres
Publié: (2025)

The Supernova 1987A system and its recent evolution - a review
par: Barlow, Michael J.
Publié: (2025)

Challenging Classical Paradigms: Recurrent Nova M31N 2017-01e, a BeWD system in M31?
par: Chamoli, Shatakshi, et autres
Publié: (2025)

LAMOST J1010+2358 is not a Pair-Instability Supernova Relic
par: Thibodeaux, Pierre N., et autres
Publié: (2024)

Astrometric microlensing probes of the isolated neutron star population with Roman
par: Kaczmarek, Zofia, et autres
Publié: (2026)

Recurrent Nova V2487 Oph Had Superflares in 1941 and 1942 With Radiant Energies 10$^{42.5\pm1.6}$ Ergs
par: Schaefer, Bradley E.
Publié: (2024)

Spectroscopic Modeling of Luminous Transients Powered by H-Rich and He-Rich Circumstellar Interaction
par: Wagle, Gururaj A., et autres
Publié: (2024)

The Crab Nebula Revisited Using HST/WFC3
par: Blair, William P., et autres
Publié: (2025)

Shell mergers in the late stages of massive star evolution: new insight from 3D hydrodynamic simulations
par: Rizzuti, Federico, et autres
Publié: (2024)

Introducing the Condor Array Telescope: III. The expansion and age of the shell of the dwarf nova Z Camelopardalis, and detection of a second, larger shell
par: Shara, Michael M., et autres
Publié: (2023)

Common Envelopes, Gamma Rays, and Sudden Spectral Changes of Novae
par: Williams, Robert, et autres
Publié: (2024)