The Color Evolution of Classical Novae. IV. Time-Stretched - and - Color-Magnitude Diagrams of Novae in Outburst
arXiv:2012.06100 · doi:10.3847/1538-4365/abd31e
Abstract
Light curves and color evolutions of two classical novae can be largely overlapped if we properly squeeze or stretch the timescale of a target nova against that of a template nova by . Then the brightness of the target nova is related to the brightness of the template nova by , where is the absolute magnitude and a function of time , and is the ratio of timescales between the target and template novae. In the previous papers of this series, we show that many novae broadly overlap in the time-stretched - color-magnitude diagram. In the present paper, we propose two other - and - diagrams, and show that their tracks overlap for 16 novae and for 52 novae, respectively. Here, , , and are the intrinsic , , and colors and not changed by the time-stretch, and , , and are the absolute , , and magnitudes. Using these properties, we considerably refine the previous estimates of their distance and reddening. The obtained distances are in reasonable agreement with those of {\it Gaia} Data Release 2 catalogue.
arXiv comment211 pages, 178 figures, typos corrected, published in ApJS, 253, 27 (2021). arXiv admin note: text overlap with arXiv:1905.10655
References in corpus (52)
- Methods and results of an automatic analysis of a complete sample of Swift-XRT observations of GRBs
- A 3D Dust Map Based on Gaia, Pan-STARRS 1 and 2MASS
- Modelling the Galactic Interstellar Extinction Distribution in Three Dimensions
- A Three-Dimensional Map of Milky-Way Dust
- Galactic Reddening in 3D from Stellar Photometry - An Improved Map
- Three-dimensional interstellar dust reddening maps of the Galactic plane
- A Universal Decline Law of Classical Novae
- Swift X-Ray Observations of Classical Novae. II. The Super Soft Source sample
- An Analytic Bolometric Light Curve Model of Interaction-Powered Supernovae and its Application to Type IIn Supernovae
- The Stony Brook / SMARTS Atlas of mostly Southern Novae
- A 3D extinction map of the Northern Galactic Plane based on IPHAS photometry
- The Distances to Novae As Seen By Gaia
- Mapping the Milky Way bulge at high resolution: the 3D dust extinction, CO, and X factor maps
- Exquisite Nova Light Curves from the Solar Mass Ejection Imager (SMEI)
- Observations of Galactic and Extragalactic Novae
- Shortest Recurrence Periods of Novae
- A Prediction Formula of Supersoft X-ray Phase of Classical Novae
- Swift X-ray Observations of Classical Novae
- Swift detection of the super-swift switch-on of the super-soft phase in nova V745 Sco (2014)
- A UV and optical study of 18 old novae with Gaia DR2 distances: mass accretion rates, physical parameters, and MMRD
- Optical and Supersoft X-ray Light Curve Models of Classical Nova V2491 Cygni: A New Clue to the Secondary Maximum
- Light Curve Analysis of Neon Novae
- The UBV Color Evolution of Classical Novae. I. Nova-Giant Sequence in the Color-Color Diagram
- The 2010 nova outburst of the symbiotic Mira V407 Cyg
- A Light Curve Analysis of Classical Novae: Free-free Emission vs. Photospheric Emission
- A New Catalogue of Galactic Novae: Investigation of the MMRD relation & Spatial Distribution
- A Light Curve Analysis of 32 Recent Galactic Novae --- Distances and White Dwarf Masses
- OGLE Atlas of Classical Novae I. Galactic Bulge Objects
- An extensive optical study of V2491 Cyg (Nova Cyg 2008 N.2), from maximum brightness to return to quiescence
- Early spectral evolution of Nova Sgr 2004 (V5114 Sgr)
- A Light Curve Analysis of Recurrent and Very Fast Novae in our Galaxy, Magellanic Clouds, and M31
- Discovery of the 2010 Eruption and the Pre-Eruption Light Curve for Recurrent Nova U Scorpii
- V496 Scuti: An Fe II nova with dust shell accompanied by CO emission
- Photometric evolution of seven recent novae and the double component characterizing the lightcurve of those emitting in gamma rays
- The UBV Color Evolution of Classical Novae. II. Color-Magnitude Diagram
- Photometric evolution, orbital modulation and progenitor of Nova Mon 2012
- Near Infrared Observations of the novae V2491 Cygni and V597 Puppis
- The nature and evolution of Nova Cygni 2006
- Evolution of the Symbiotic Nova PU Vul -- Outbursting White Dwarf, Nebulae, and Pulsating Red Giant Companion
- The luminosity evolution of nova shells -- I. A new analysis of old data
- The Distances of the Galactic Novae
- Near Infrared studies during maximum and early decline of Nova Cephei 2014 and Nova Scorpii 2015
- A Theory for the Maximum Magnitude versus Rate of Decline (MMRD) Relation of Classical Novae
- Nova light curves from the Solar Mass Ejection Imager (SMEI) - II. The extended catalog
- The 2010 Eruption of the Recurrent Nova U Scorpii: The Multi-Wavelength Light Curve
- The Color Evolution of Classical Novae. III. Time-Stretched Color-Magnitude Diagram of Novae in Outburst
- Optical evolution of Nova Ophiuchi 2007 = V2615 Oph
- A Light Curve Analysis of Gamma-ray Nova V959 Mon -- Distance and White Dwarf Mass
- Multiwavelength modeling the SED of nova V339~Del: Stopping the wind and long-lasting super-Eddington luminosity with dust emission
- ASASSN-16oh: A nova outburst with no mass ejection -- A new type of supersoft X-ray source in old populations
- Supersoft X-Ray Phases of Recurrent Novae as an Indicator of their White Dwarf Masses
- Optical and Near-Infrared Photometry of Nova V2362 Cyg : Rebrightening Event and Dust Formation
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- Comprehensive Catalogue of the Overall Best Distances and Properties of 402 Galactic Novae
- A strong shock during a nova outburst: an origin of multiple velocity systems in optical spectra and of high-energy emissions
- Physics of nova outbursts: A theoretical model of classical nova outbursts with self-consistent wind mass loss
- A multiwavelength light curve analysis of the classical nova YZ Ret: An extension of the universal decline law to the nebular phase
- A light curve model of V2491 Cyg: Classical nova outburst on a cool and massive white dwarf