A comprehensive light curve model of the very fast nova V1674 Herculis
Fuente:
arXiv
Saved in:
| Main Authors: | Kato, Mariko, Hachisu, Izumi, Saio, Hideyuki |
|---|---|
| Format: | Preprint |
| Published: |
2025
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
Fully self-consistent nova explosion models reproducing light curves of KT Eri, V339 Del, V597 Pup, and SMC NOVA 2016-10a
by: Kato, Mariko, et al.
Published: (2025)
by: Kato, Mariko, et al.
Published: (2025)
Formation of an optically thick shocked shell in the very fast nova V1674 Herculis: the origin of superbrightness
by: Hachisu, Izumi, et al.
Published: (2025)
by: Hachisu, Izumi, et al.
Published: (2025)
Optical detection of the X-ray flash in the very fast nova V1674 Her: Optical contribution of the irradiated accretion disk
by: Hachisu, Izumi, et al.
Published: (2025)
by: Hachisu, Izumi, et al.
Published: (2025)
Physics of nova outbursts: Theoretical models of classical nova outbursts with optically thick winds on $1.2~M_\odot$ and $1.3~M_\odot$ white dwarfs
by: Kato, Mariko, et al.
Published: (2024)
by: Kato, Mariko, et al.
Published: (2024)
A multiwavelength light curve analysis of the classical nova V392 Per: Optical contribution from an irradiated accretion disk during the nova wind phase
by: Hachisu, Izumi, et al.
Published: (2025)
by: Hachisu, Izumi, et al.
Published: (2025)
A multiwavelength light curve model of the classical nova V339 Del: A mechanism for the coexistence of dust dip and supersoft X-rays
by: Hachisu, Izumi, et al.
Published: (2024)
by: Hachisu, Izumi, et al.
Published: (2024)
Upper bound of ejecta mass in a nova outburst
by: Hachisu, Izumi, et al.
Published: (2026)
by: Hachisu, Izumi, et al.
Published: (2026)
Optical observations of the fast nova V1674 Herculis
by: Rawat, Neeraj Singh, et al.
Published: (2026)
by: Rawat, Neeraj Singh, et al.
Published: (2026)
A multiwavelength light curve analysis of the classical nova KT Eri: Optical contribution from a large irradiated accretion disk
by: Hachisu, Izumi, et al.
Published: (2024)
by: Hachisu, Izumi, et al.
Published: (2024)
A demarcation criterion for hydrogen burning of millinovae
by: Hachisu, Izumi, et al.
Published: (2025)
by: Hachisu, Izumi, et al.
Published: (2025)
X-Ray Flashes on Helium Novae
by: Kato, Mariko, et al.
Published: (2024)
by: Kato, Mariko, et al.
Published: (2024)
The Rise of Nova V1674 Herculis
by: Quimby, Robert M., et al.
Published: (2024)
by: Quimby, Robert M., et al.
Published: (2024)
The orbital period of the nova V1674 Her as observed with TESS
by: Luna, G. J. M., et al.
Published: (2023)
by: Luna, G. J. M., et al.
Published: (2023)
Pulsating B stars in the Scorpius-Centaurus Association with TESS
by: Sharma, Awshesh N., et al.
Published: (2022)
by: Sharma, Awshesh N., et al.
Published: (2022)
On the light-curves of disk and bulge novae
by: Cohen, Asaf, et al.
Published: (2025)
by: Cohen, Asaf, et al.
Published: (2025)
Asteroseismic detection of a predominantly toroidal magnetic field in the deep interior of the main-sequence F star KIC 9244992
by: Takata, Masao, et al.
Published: (2025)
by: Takata, Masao, et al.
Published: (2025)
Linear adiabatic analysis for general relativistic instability in primordial accreting supermassive stars
by: Saio, Hideyuki, et al.
Published: (2024)
by: Saio, Hideyuki, et al.
Published: (2024)
Magnetic activity under tidal influences in the 2+2~hierarchical quadruple system V815 Herculis
by: Kővári, Zs., et al.
Published: (2024)
by: Kővári, Zs., et al.
Published: (2024)
The $μ$ Herculis system solved after nearly three centuries
by: Marcussen, Marcus L., et al.
Published: (2026)
by: Marcussen, Marcus L., et al.
Published: (2026)
A TESS View of Post-Eruption Variability in the Novae V1405 Cas,V1716 Sco, and V1674 Her
by: Luna, G. J. M., et al.
Published: (2025)
by: Luna, G. J. M., et al.
Published: (2025)
Glitch analysis and asteroseismic modelling of subgiant $μ$ Herculis: confirming and interpreting the $Γ_1$ peak as the helium glitch
by: Gupta, Advik, et al.
Published: (2025)
by: Gupta, Advik, et al.
Published: (2025)
The 2021 Hot-type Symbiotic Outburst of YY Herculis: An Optical Follow-up Study
by: Sonith, L. S., et al.
Published: (2026)
by: Sonith, L. S., et al.
Published: (2026)
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)
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)
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)
X-ray spectroscopy mass constraints on V1674 Her: the fastest nova does not have a near-Chandrasekhar white dwarf
by: Olbemo, Tekeba, et al.
Published: (2026)
by: Olbemo, Tekeba, et al.
Published: (2026)
The EBLM project -- XIV. TESS light curves for eclipsing binaries with very low mass companions
by: Fitzpatrick, Jay, et al.
Published: (2025)
by: Fitzpatrick, Jay, et al.
Published: (2025)
HD 12098: a highly distorted dipole mode in an obliquely pulsating roAp star
by: Kurtz, D. W., et al.
Published: (2024)
by: Kurtz, D. W., et al.
Published: (2024)
The model fitting of Gaia DR3 Classical Cepheid light and radial velocity curves
by: Molinaro, R., et al.
Published: (2025)
by: Molinaro, R., et al.
Published: (2025)
Apsidal motion and TESS light curves of two southern eclipsing binaries with high eccentricity: V1647 Sgr and V2283 Sgr
by: Wolf, Marek, et al.
Published: (2026)
by: Wolf, Marek, et al.
Published: (2026)
ASASSN-24hd; a dwarf nova bridging WZ Sge-type and SU UMa-type superoutbursts
by: Tampo, Yusuke, et al.
Published: (2025)
by: Tampo, Yusuke, et al.
Published: (2025)
The light curve model fitting of LMC Cepheids: MESA-RSP versus Stellingwerf's code predictions
by: Deka, M., et al.
Published: (2025)
by: Deka, M., et al.
Published: (2025)
Detection and analysis of white-light emission in solar flares through light curve diagnostics
by: Li, Shuanghong, et al.
Published: (2026)
by: Li, Shuanghong, et al.
Published: (2026)
Classifying the derivatives of light curves for overcontact eclipsing binaries
by: Kouzuma, Shinjirou
Published: (2025)
by: Kouzuma, Shinjirou
Published: (2025)
A probable inside-out dwarf nova outburst from the period bouncer candidate ASASSN-25dc
by: Tampo, Yusuke, et al.
Published: (2026)
by: Tampo, Yusuke, et al.
Published: (2026)
The massive binary system WR 20a: light curve analysis in a colliding wind model
by: Antokhin, I. I., et al.
Published: (2025)
by: Antokhin, I. I., et al.
Published: (2025)
Nebular Nitrogen Line Emission in Stripped-Envelope Supernovae -- a New Progenitor Mass Diagnostic
by: Barmentloo, Stan, et al.
Published: (2024)
by: Barmentloo, Stan, et al.
Published: (2024)
Exploring the connection between atmosphere models and evolution models of very massive stars
by: Josiek, Joris, et al.
Published: (2025)
by: Josiek, Joris, et al.
Published: (2025)
A dusty rain falls on the nova V959 Monocerotis
by: Evans, A., et al.
Published: (2024)
by: Evans, A., et al.
Published: (2024)
A very young and fast rotating shell star discovered in the eclipsing binary ZTF J200347.63+394429.8
by: Hauck, Norbert
Published: (2025)
by: Hauck, Norbert
Published: (2025)
Similar Items
-
Fully self-consistent nova explosion models reproducing light curves of KT Eri, V339 Del, V597 Pup, and SMC NOVA 2016-10a
by: Kato, Mariko, et al.
Published: (2025) -
Formation of an optically thick shocked shell in the very fast nova V1674 Herculis: the origin of superbrightness
by: Hachisu, Izumi, et al.
Published: (2025) -
Optical detection of the X-ray flash in the very fast nova V1674 Her: Optical contribution of the irradiated accretion disk
by: Hachisu, Izumi, et al.
Published: (2025) -
Physics of nova outbursts: Theoretical models of classical nova outbursts with optically thick winds on $1.2~M_\odot$ and $1.3~M_\odot$ white dwarfs
by: Kato, Mariko, et al.
Published: (2024) -
A multiwavelength light curve analysis of the classical nova V392 Per: Optical contribution from an irradiated accretion disk during the nova wind phase
by: Hachisu, Izumi, et al.
Published: (2025)