Chomiuk, L., Metzger, BD & Shen, KJ New perspectives on classical novae. Ann. Reverend Astron. Astrophysic. 59391-444 (2021).
Starrfield, S., Iliadis, C. & Hix, WR Thermonuclear runaway and the classic nova explosion. Publ. Star. Soc. Peaceful 128051001 (2016).
Google Scholar
Hillman, Y., Prialnik, D., Kovetz, A., Shara, MM & Neill, JD Nova Multi-Wavelength Light Curves: Prediction of UV Precursor Flashes and Pre-Maximum Arrests. Mon. No. R.Astron. Soc. 4371962-1975 (2014).
Google Scholar
Starrfield, S., Truran, JW, Sparks, WM, Krautter, J. & MacDonald, J. in Physics of classical novae (eds Cassatella, A. & Viotti, R.) 306–310 (Springer, 1990).
Krautter, J. in RS Ophiuchi (2006) and the recurring Nova phenomenon (eds Evans, A. et al.) Astron. Soc. Conf. Pacific Ser 401, 139 (Astronomical Society of the Pacific, 2008).
Kato, M., Saio, H. & Hachisu, I. Nova M31N 2008-12A one-year return period multi-wavelength light curve model. Astrophysic. J 80852 (2015).
Google Scholar
Kato, M. et al. X-ray flashes in recurrent novae: M31N 2008-12a and the implications of Swift’s non-detection. Astrophysic. J 83040 (2016).
Google Scholar
Morii, M., Yamaoka, H., Mihara, T., Matsuoka, M., and Kawai, N. Searching for soft X-rays during the fireball phase of classical/recurrent novae using MAXI/ GSC. Publ. Star. Soc. Japan 68S11 (2016).
Google Scholar
Predehl, P. et al. The eROSITA X-ray telescope on SRG. Star. Astrophysic. 647A1 (2021).
Google Scholar
Sunyaev, R. et al. SRG X-ray orbital observatory. His telescopes and his first scientific results. Star. Astrophysic. 656A132 (2021).
Google Scholar
McNaught, RH Nova apparent in the reticulum. CBET 4811 (2020).
Aydi, E. et al. SALT spectroscopic classification of MGAB-V207 as a classical nova. ATEL 13867 (2020).
Carr, A., Said, K., Davis, TM, Lidman, C. & Tucker, BE WiFeS tracking observations of the naked-eye nova associated with MGAB-V207. ATEL13874 (2020).
Sokolovsky, KV et al. NuSTAR detection of Nova Reticuli 2020 = MGAB-V207. ATEL 13900 (2020).
McNaught, RH Nova Reticuli 2020. CBET 4812 (2020).
Li, K.-L. et al. Fermi-LAT detection of classical nova with the naked eye MGAB-V207. ATEL 13868 (2020).
Sokolovsky, KV et al. The first nova flare in a nova-like variable: YZ Ret seen in X-rays and gamma rays. Preprint at https://arxiv.org/abs/2108.03241 (2021).
Kilkenny, D. et al. The Edinburgh-Cape Blue Object Survey – IV. Zone 3: Galactic latitudes –40° > b > –50°. Mon. No. R.Astron. Soc. 4531879–1887 (2015).
Google Scholar
Schaefer, BE Discovery of 13 new orbital periods for classical novae. Res. Remarks American Astro. Soc. 5150 (2021).
Google Scholar
Dauser, T. et al. SIXTE: a generic X-ray instrument simulation toolbox. Star. Astrophysic. 630A66 (2019).
Google Scholar
Smith, RK, Brickhouse, NS, Liedahl, DA & Raymond, JC Collision plasma models with APEC/APED: emission line diagnosis of hydrogen and helium-like ions. Astrophysic. J 556L91–L95 (2001).
Google Scholar
Suleimanov, VF, Mauche, CW, Zhuchkov, RY, and Werner, K. Fitting the Chandra LETG spectrum of exploding SS Cygni with model atmosphere spectra in 18th European White Dwarf Workshop Flight. 469 (eds Krzesiński, J. et al.) 349 (Astronomical Society of the Pacific, 2013).
Suleimanov, V., Hertfelder, M., Werner, K. & Kley, W. Modeling EUV spectra of optically thick boundary layers of exploding dwarf novae. Star. Astrophysic. 571A55 (2014).
Google Scholar
Izzo, L. et al. UVES observations of Nova Reticuli 2020 during minimal science operations show that it is entering the nebular phase. ATEL 14048 (2020).
José, J. & Hernanz, M. Nucleosynthesis in classical novae: CO versus ONe white dwarfs. Astrophysic. J 494680–690 (1998).
Google Scholar
Aydi, E. et al. Early spectral evolution of classical novae: consistent evidence for several distinct outflows. Astrophysic. J 90562 (2020).
Google Scholar
Bédard, A., Bergeron, P. & Fontaine, G. Measurements of the physical parameters of white dwarfs: a test of the mass-radius relationship. Astrophysic. J 84811 (2017).
Google Scholar
Sokolovsky, K. et al. Super soft x-ray emission from Nova Reticuli 2020. ATEL 14043 (2020).
Kato, M., Saio, H. & Hachisu, I. A self-consistent model for a full cycle of recurrent novaewind mass loss rate and X-ray luminosity. Astrophysic. J 838153 (2017).
Google Scholar
Cao, Y. et al. Classic Novae in Andromeda: Palomar Transient Factory and GALEX light curves. Astrophysic. J 752133 (2012).
Google Scholar
Pietsch, W., Sala, G., Haberl, F. & Greiner, J. M31N 2007-07c nova detection with Swift UVOT in UVW2 filter. ATEL 1149 (2007).
De, K. et al. A population of strongly reddened and optically missed Palomar Gattini-IR novae: constraints on the galactic nova rate. Astrophysic. J 91219 (2021).
Google Scholar
Wilms, J., Allen, A. & McCray, R. On the absorption of X-rays in the interstellar medium. Astrophysic. J 542914–924 (2000).
Google Scholar
Verner, DA, Ferland, GJ, Korista, KT & Yakovlev, DG Atomic Data for Astrophysics. II. New analytical FITS for photoionization cross sections of atoms and ions. Astrophysic. J 465487 (1996).
Google Scholar
Ballet, J. Pile-up on CCD X-ray instruments. Star. Astrophysic. Sup. 135371–381 (1999).
Google Scholar
Davis, JE Event accumulation in charge-coupled devices. Astrophysic. J 562575–582 (2001).
Google Scholar
Tamba, T. et al. Spectral analysis based on simulation of X-ray CCD data affected by photon stacking. Publ. Star. Soc. Japan 74364-383 (2021).
Lampton, M., Margon, B. & Bowyer, S. Parameter estimation in X-ray astronomy. Astrophysic. J 208177-190 (1976).
Google Scholar
Townsley, LK et al. CCD simulation for the Chandra Advanced CCD imaging spectrometer. Nucl. Inst. Physical methods. Res. A 486716–750 (2002).
Google Scholar
Seaton, MJ, Yan, Y., Mihalas, D. & Pradhan, AK Opacities for Stellar Envelopes. Mon. No. R.Astron. Soc. 266805 (1994).
Google Scholar
Dere, KP, Landi, E., Mason, HE, Monsignori Fossi, BC & Young, PR CHIANTI – an atomic database for emission lines. Star. Astrophysic. Supplement 125149-173 (1997).
Google Scholar
Kochanek, CS et al. The All-Sky Automated Survey for Supernovae (ASAS-SN) lightcurve server v1.0. Publ. Star. Soc. Peaceful 129104502 (2017).
Google Scholar
Pei, S. et al. NICER observations from Nova Ret 2020. ATEL 14067 (2020).
Drake, JJ et al. Chandra High Resolution X-ray Spectroscopy from Nova Ret 2020. ATEL 14214 (2020).
Atwood, WB et al. The Large Area Telescope of the Fermi Space Telescope Gamma-Ray mission. Astrophysic. J 6971071-1102 (2009).
Google Scholar
Wood, M. et al. Fermipy: an open-source Python package for analyzing Fermi-LAT data in 35th International Conference on Cosmic Rays (ICRC2017) (eds. Il Heung Park et al.) 301, 824 (Proceedings of Science, 2017).
Cash, W. Parameter estimation in astronomy by applying the likelihood ratio. Astrophysic. J 228939–947 (1979).
Google Scholar
Dennerl, K. et al. Determination of the half-energy width (HEW) of the eROSITA mirror with sub-pixel resolution in Space telescopes and instrumentation 2012: from ultraviolet to gamma rays Flight. 8443 (eds Takahashi, T. et al.) 844350 (SPIE, 2012).