Chomiuk, L., Metzger, B. D. & Shen, Okay. J. New insights into classical novae. Annu. Rev. Astron. Astrophys. 59, 391-444 (2021).
Starrfield, S., Iliadis, C. & Hix, W. R. The thermonuclear runaway and the classical nova outburst. Publ. Astron. Soc. Pacific 128, 051001 (2016).
Google Scholar
Hillman, Y., Prialnik, D., Kovetz, A., Shara, M. M. & Neill, J. D. Nova multiwavelength gentle curves: predicting UV precursor flashes and pre-maximum halts. Mon. Not. R. Astron. Soc. 437, 1962–1975 (2014).
Google Scholar
Starrfield, S., Truran, J. W., Sparks, W. M., 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 Recurrent Nova Phenomenon (eds Evans, A. et al.) Astron. Soc. Pacific Conf. Ser 401, 139 (Astronomical Society of the Pacific, 2008).
Kato, M., Saio, H. & Hachisu, I. Multi-wavelength gentle curve mannequin of the one-year recurrence interval Nova M31N 2008-12A. Astrophys. J. 808, 52 (2015).
Google Scholar
Kato, M. et al. X-ray flashes in recurrent novae: M31N 2008-12a and the implications of the Swift nondetection. Astrophys. J. 830, 40 (2016).
Google Scholar
Morii, M., Yamaoka, H., Mihara, T., Matsuoka, M. & Kawai, N. Search for mushy X-ray flashes at the fireball phase of classical/recurrent novae utilizing MAXI/GSC knowledge. Publ. Astron. Soc. Japan 68, S11 (2016).
Google Scholar
Predehl, P. et al. The eROSITA X-ray telescope on SRG. Astron. Astrophys. 647, A1 (2021).
Google Scholar
Sunyaev, R. et al. SRG X-ray orbital observatory. Its telescopes and first scientific outcomes. Astron. Astrophys. 656, A132 (2021).
Google Scholar
McNaught, R. H. Apparent nova in Reticulum. CBET 4811 (2020).
Aydi, E. et al. SALT spectroscopic classification of MGAB-V207 as a classical nova. ATeL 13867 (2020).
Carr, A., Said, Okay., Davis, T. M., Lidman, C. & Tucker, B. E. WiFeS follow-up observations of the naked-eye nova related to MGAB-V207. ATeL13874 (2020).
Sokolovsky, Okay. V. et al. NuSTAR detection of Nova Reticuli 2020 = MGAB-V207. ATeL 13900 (2020).
McNaught, R. H. Nova Reticuli 2020. CBET 4812 (2020).
Li, Okay.-L. et al. Fermi-LAT detection of the naked-eye classical nova MGAB-V207. ATeL 13868 (2020).
Sokolovsky, Okay. V. et al. The first nova eruption in a novalike variable: YZ Ret as 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. Not. R. Astron. Soc. 453, 1879–1887 (2015).
Google Scholar
Schaefer, B. E. Discovery of 13 new orbital intervals for classical novae. Res. Notes American Astron. Soc. 5, 150 (2021).
Google Scholar
Dauser, T. et al. SIXTE: a generic X-ray instrument simulation toolkit. Astron. Astrophys. 630, A66 (2019).
Google Scholar
Smith, R. Okay., Brickhouse, N. S., Liedahl, D. A. & Raymond, J. C. Collisional plasma fashions with APEC/APED: emission-line diagnostics of hydrogen-like and helium-like ions. Astrophys. J. 556, L91–L95 (2001).
Google Scholar
Suleimanov, V. F., Mauche, C. W., Zhuchkov, R. Y. & Werner, Okay. Fitting the Chandra LETG Spectrum of SS Cygni in Outburst with Model Atmosphere Spectra in 18th European White Dwarf Workshop Vol. 469 (eds Krzesiński, J. et al.) 349 (Astronomical Society of the Pacific, 2013).
Suleimanov, V., Hertfelder, M., Werner, Okay. & Kley, W. Modeling the EUV spectra of optically thick boundary layers of dwarf novae in outburst. Astron. Astrophys. 571, A55 (2014).
Google Scholar
Izzo, L. et al. UVES observations of Nova Reticuli 2020 throughout minimal science operations present it’s getting into the nebular phase. ATeL 14048 (2020).
José, J. & Hernanz, M. Nucleosynthesis in classical novae: CO versus ONe white dwarfs. Astrophys. J. 494, 680–690 (1998).
Google Scholar
Aydi, E. et al. Early spectral evolution of classical novae: constant proof for a number of distinct outflows. Astrophys. J. 905, 62 (2020).
Google Scholar
Bédard, A., Bergeron, P. & Fontaine, G. Measurements of bodily parameters of white dwarfs: a check of the mass-radius relation. Astrophys. J. 848, 11 (2017).
Google Scholar
Sokolovsky, Okay. et al. Super-soft X-ray emission of Nova Reticuli 2020. ATeL 14043 (2020).
Kato, M., Saio, H. & Hachisu, I. A self-consistent mannequin for a full cycle of recurrent novaewind mass-loss price and x-ray luminosity. Astrophys. J. 838, 153 (2017).
Google Scholar
Cao, Y. et al. Classical novae in Andromeda: gentle curves from the Palomar Transient Factory and GALEX. Astrophys. J. 752, 133 (2012).
Google Scholar
Pietsch, W., Sala, G., Haberl, F. & Greiner, J. Detection of nova M31N 2007-07c with Swift UVOT in the UVW2 filter. ATEL 1149 (2007).
De, Okay. et al. A inhabitants of closely reddened, optically missed novae from Palomar Gattini-IR: constraints on the galactic nova price. Astrophys. J. 912, 19 (2021).
Google Scholar
Wilms, J., Allen, A. & McCray, R. On the absorption of x-rays in the interstellar medium. Astrophys. J. 542, 914–924 (2000).
Google Scholar
Verner, D. A., Ferland, G. J., Korista, Okay. T. & Yakovlev, D. G. Atomic knowledge for astrophysics. II. New Analytic FITS for photoionization cross sections of atoms and ions. Astrophys. J. 465, 487 (1996).
Google Scholar
Ballet, J. Pile-up on X-ray CCD devices. Astron. Astrophys. Supp. 135, 371–381 (1999).
Google Scholar
Davis, J. E. Event pileup in charge-coupled units. Astrophys. J. 562, 575–582 (2001).
Google Scholar
Tamba, T. et al. Simulation-based spectral evaluation of X-ray CCD knowledge affected by photon pile-up. Publ. Astron. Soc. Japan 74, 364-383 (2021).
Lampton, M., Margon, B. & Bowyer, S. Parameter estimation in X-ray astronomy. Astrophys. J. 208, 177–190 (1976).
Google Scholar
Townsley, L. Okay. et al. Simulating CCDs for the Chandra Advanced CCD Imaging Spectrometer. Nucl. Inst. Methods Phys. Res. A 486, 716–750 (2002).
Google Scholar
Seaton, M. J., Yan, Y., Mihalas, D. & Pradhan, A. Okay. Opacities for stellar envelopes. Mon. Not. R. Astron. Soc. 266, 805 (1994).
Google Scholar
Dere, Okay. P., Landi, E., Mason, H. E., Monsignori Fossi, B. C. & Young, P. R. CHIANTI – an atomic database for emission traces. Astron. Astrophys. Suppl. 125, 149–173 (1997).
Google Scholar
Kochanek, C. S. et al. The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server v1.0. Publ. Astron. Soc. Pacific 129, 104502 (2017).
Google Scholar
Pei, S. et al. NICER observations of Nova Ret 2020. ATeL 14067 (2020).
Drake, J. J. et al. Chandra excessive decision X-ray spectroscopy of Nova Ret 2020. ATeL 14214 (2020).
Atwood, W. B. et al. The Large Area Telescope on the Fermi Gamma-Ray Space Telescope Mission. Astrophys. J. 697, 1071–1102 (2009).
Google Scholar
Wood, M. et al. Fermipy: An open-source Python package deal for evaluation of Fermi-LAT Data in thirty fifth International Cosmic Ray Conference (ICRC2017) (eds. Il Heung Park et al.) 301, 824 (Proceedings of Science, 2017).
Cash, W. Parameter estimation in astronomy by utility of the probability ratio. Astrophys. J. 228, 939–947 (1979).
Google Scholar
Dennerl, Okay. et al. Determination of the eROSITA mirror half power width (HEW) with subpixel decision in Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray Vol. 8443 (eds Takahashi, T. et al.) 844350 (SPIE, 2012).
X-ray detection of a nova in the fireball phase & More Latest News Update
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