Modeling the high-brightness state of the recurrent nova T CrB as an enhanced mass-transfer event
Fuente:
arXiv
Saved in:
| Main Authors: | Schlindwein, Wagner, Baptista, Raymundo, Luna, Gerardo Juan Manuel |
|---|---|
| Format: | Preprint |
| Published: |
2025
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
The accretion-driven eruption of the recurrent nova T Corona Borealis
by: Baptista, Raymundo, et al.
Published: (2026)
by: Baptista, Raymundo, et al.
Published: (2026)
Evolution of the recent high-accretion state of the recurrent nova T CrB: HST, Swift, NuSTAR, and XMM-Newton observations
by: Luna, G. J. M., et al.
Published: (2026)
by: Luna, G. J. M., et al.
Published: (2026)
The pre-eruption state of T CrB as observed with ALMA in 2024
by: Petry, D., et al.
Published: (2025)
by: Petry, D., et al.
Published: (2025)
Mass-transfer Outburts reborn: Modeling the light curve of the dwarf nova EX Draconis
by: Schlindwein, Wagner, et al.
Published: (2024)
by: Schlindwein, Wagner, et al.
Published: (2024)
Evolution of the optical emission lines and the X-ray emission during the super-active stage of T CrB
by: Stoyanov, K. A., et al.
Published: (2024)
by: Stoyanov, K. A., et al.
Published: (2024)
The dwarf nova EX Draconis: a short review
by: Baptista, Raymundo, et al.
Published: (2026)
by: Baptista, Raymundo, et al.
Published: (2026)
Analysis of optical spectroscopy and photometry of the type I X-ray bursting system UW CrB
by: Kennedy, M. R., et al.
Published: (2024)
by: Kennedy, M. R., et al.
Published: (2024)
Is the Symbiotic Recurrent Nova T CrB Late? Recent Photometric Evolution and Comparison with Past Pre-Outburst Behaviour
by: Merc, Jaroslav, et al.
Published: (2025)
by: Merc, Jaroslav, et al.
Published: (2025)
Size of the accretion disc in the recurrent nova T CrB
by: Zamanov, R. K., et al.
Published: (2024)
by: Zamanov, R. K., et al.
Published: (2024)
Ancient nova shells of RX Pup indicate evolution of mass transfer rate
by: Ilkiewicz, Krystian, et al.
Published: (2024)
by: Ilkiewicz, Krystian, et al.
Published: (2024)
Exploring extreme brightness variations in blue supergiant MACHO 80.7443.1718: Evidence for companion-driven enhanced mass loss
by: Kołaczek-Szymański, Piotr Antoni, et al.
Published: (2023)
by: Kołaczek-Szymański, Piotr Antoni, et al.
Published: (2023)
Identification of recurrent novae from parametric modeling of the optical light curve
by: Barman, Rajarshi, et al.
Published: (2025)
by: Barman, Rajarshi, et al.
Published: (2025)
Multi-wavelength study of the pre-eruption dip in the recurrent nova T Coronae Borealis preceding imminent nova eruption
by: Pei, Songpeng, et al.
Published: (2025)
by: Pei, Songpeng, et al.
Published: (2025)
Pre-outburst signal in the light curves of the recurrent novae RS Oph and T CrB
by: Zamanov, R. K., et al.
Published: (2023)
by: Zamanov, R. K., et al.
Published: (2023)
Interaction between the ejecta, the accretion disk, and the secondary star in the recurrent nova system U Sco
by: Figueira, Joana, et al.
Published: (2026)
by: Figueira, Joana, et al.
Published: (2026)
On the effects of radiation on mass transfer in binary stars
by: Cehula, Jakub, et al.
Published: (2025)
by: Cehula, Jakub, et al.
Published: (2025)
Exploring mass transfer mechanisms in symbiotic systems
by: Vathachira, Irin Babu, et al.
Published: (2025)
by: Vathachira, Irin Babu, et al.
Published: (2025)
Multi-wavelength observations of multiple eruptions of the recurrent nova M31N 2008-12a
by: Basu, Judhajeet, et al.
Published: (2023)
by: Basu, Judhajeet, et al.
Published: (2023)
Upper bound of ejecta mass in a nova outburst
by: Hachisu, Izumi, et al.
Published: (2026)
by: Hachisu, Izumi, et al.
Published: (2026)
The slowest spinning Galactic-field spider PSR J1932+2121: A history of inefficient mass transfer
by: Misra, Devina, et al.
Published: (2025)
by: Misra, Devina, et al.
Published: (2025)
Interacting supernovae from wide mass-transferring binaries
by: Ercolino, Andrea
Published: (2024)
by: Ercolino, Andrea
Published: (2024)
Understanding the impact of binary mass transfer in the accretor's measurable parameters
by: Vilaxa-Campos, Magdalena, et al.
Published: (2026)
by: Vilaxa-Campos, Magdalena, et al.
Published: (2026)
Forming merging double compact objects with stable mass transfer
by: Picco, Annachiara, et al.
Published: (2023)
by: Picco, Annachiara, et al.
Published: (2023)
WR + O binaries as probes of the first phase of mass transfer
by: Nuijten, Marit, et al.
Published: (2024)
by: Nuijten, Marit, et al.
Published: (2024)
Binary mass transfer in 3D: Mass Transfer Rate and Morphology
by: Ryu, T., et al.
Published: (2025)
by: Ryu, T., et al.
Published: (2025)
Expansion of accreting main-sequence stars during rapid mass transfer
by: Lau, Mike Y. M., et al.
Published: (2024)
by: Lau, Mike Y. M., et al.
Published: (2024)
Rapid binary mass transfer: Circumbinary outflows and angular momentum losses
by: Scherbak, Peter, et al.
Published: (2025)
by: Scherbak, Peter, et al.
Published: (2025)
Theoretical expectations for high-mass X-ray binaries, supernova remnants, and their evolutionary paths: An overview talk for LIAC41: the eventful life of stellar multiples
by: Mandel, Ilya
Published: (2024)
by: Mandel, Ilya
Published: (2024)
V407 Lup, an intermediate polar nova
by: Orio, M., et al.
Published: (2024)
by: Orio, M., et al.
Published: (2024)
Irradiation-driven mass transfer for massive companion stars in supersoft X-rays sources
by: Zhao, Weitao, et al.
Published: (2024)
by: Zhao, Weitao, et al.
Published: (2024)
Coping with loss: Stability of mass transfer from post-main sequence donor stars
by: Temmink, K. D., et al.
Published: (2022)
by: Temmink, K. D., et al.
Published: (2022)
Observational diversity of bright long-lived Type II supernovae
by: Nagao, T., et al.
Published: (2025)
by: Nagao, T., et al.
Published: (2025)
X-ray spectropolarimetry of the bright atoll Serpens X-1
by: Ursini, F., et al.
Published: (2024)
by: Ursini, F., et al.
Published: (2024)
Search for GeV gamma-ray emission from the possible TeV-bright red dwarfs with Fermi-LAT
by: Huang, Chen, et al.
Published: (2024)
by: Huang, Chen, et al.
Published: (2024)
Expanding the ultracompacts: gravitational wave-driven mass transfer in the shortest-period binaries with accretion disks
by: Chakraborty, Joheen, et al.
Published: (2024)
by: Chakraborty, Joheen, et al.
Published: (2024)
Population synthesis of Be X-ray binaries in the Small Magellanic Cloud: angular momentum recycling and stable mass transfer
by: Oller, Víctor López, et al.
Published: (2026)
by: Oller, Víctor López, et al.
Published: (2026)
Symbiotic novae
by: Munari, Ulisse
Published: (2024)
by: Munari, Ulisse
Published: (2024)
HD3191, the high-mass X-ray binary that wasn't there
by: Rauw, Gregor, et al.
Published: (2026)
by: Rauw, Gregor, et al.
Published: (2026)
Enabling high mass accretion rates onto massive main sequence stars by outer envelope mass removal
by: Scolnic, Ariel, et al.
Published: (2025)
by: Scolnic, Ariel, et al.
Published: (2025)
Analytic approximations for massive close post-mass transfer binary systems
by: Schürmann, Christoph, et al.
Published: (2024)
by: Schürmann, Christoph, et al.
Published: (2024)
Similar Items
-
The accretion-driven eruption of the recurrent nova T Corona Borealis
by: Baptista, Raymundo, et al.
Published: (2026) -
Evolution of the recent high-accretion state of the recurrent nova T CrB: HST, Swift, NuSTAR, and XMM-Newton observations
by: Luna, G. J. M., et al.
Published: (2026) -
The pre-eruption state of T CrB as observed with ALMA in 2024
by: Petry, D., et al.
Published: (2025) -
Mass-transfer Outburts reborn: Modeling the light curve of the dwarf nova EX Draconis
by: Schlindwein, Wagner, et al.
Published: (2024) -
Evolution of the optical emission lines and the X-ray emission during the super-active stage of T CrB
by: Stoyanov, K. A., et al.
Published: (2024)