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Hachisu, Izumi, Kato, Mariko (2009) OPTICAL AND SUPERSOFT X-RAY LIGHT-CURVE MODELS OF CLASSICAL NOVA V2491 CYGNI: A NEW CLUE TO THE SECONDARY MAXIMUM. The Astrophysical Journal, 694 (2). doi:10.1088/0004-637x/694/2/l103

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Reference TypeJournal (article/letter/editorial)
TitleOPTICAL AND SUPERSOFT X-RAY LIGHT-CURVE MODELS OF CLASSICAL NOVA V2491 CYGNI: A NEW CLUE TO THE SECONDARY MAXIMUM
JournalThe Astrophysical Journal
AuthorsHachisu, IzumiAuthor
Kato, MarikoAuthor
Year2009 (April 1)Volume694
Issue2
PublisherIOP Publishing
DOIdoi:10.1088/0004-637x/694/2/l103Search in ResearchGate
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Mindat Ref. ID3372835Long-form Identifiermindat:1:5:3372835:7
GUID0
Full ReferenceHachisu, Izumi, Kato, Mariko (2009) OPTICAL AND SUPERSOFT X-RAY LIGHT-CURVE MODELS OF CLASSICAL NOVA V2491 CYGNI: A NEW CLUE TO THE SECONDARY MAXIMUM. The Astrophysical Journal, 694 (2). doi:10.1088/0004-637x/694/2/l103
Plain TextHachisu, Izumi, Kato, Mariko (2009) OPTICAL AND SUPERSOFT X-RAY LIGHT-CURVE MODELS OF CLASSICAL NOVA V2491 CYGNI: A NEW CLUE TO THE SECONDARY MAXIMUM. The Astrophysical Journal, 694 (2). doi:10.1088/0004-637x/694/2/l103
In(2009, April) The Astrophysical Journal Vol. 694 (2) IOP Publishing

See Also

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Hachisu, Izumi, Kato, Mariko (2010) A PREDICTION FORMULA OF SUPERSOFT X-RAY PHASE OF CLASSICAL NOVAE. The Astrophysical Journal, 709 (2). 680-714 doi:10.1088/0004-637x/709/2/680
Hachisu, Izumi, Kato, Mariko (2014) A LIGHT CURVE ANALYSIS OF CLASSICAL NOVAE: FREE-FREE EMISSION VERSUS PHOTOSPHERIC EMISSION. The Astrophysical Journal, 798 (2). 76pp. doi:10.1088/0004-637x/798/2/76
Hachisu, Izumi, Kato, Mariko, Luna, Gerardo Juan Manuel (2007) Supersoft X-Ray Light Curve of RS Ophiuchi (2006). The Astrophysical Journal, 659 (2). doi:10.1086/516838
Hachisu, Izumi, Kato, Mariko (2005) Toward a Unified Light‐Curve Model for Multiwavelength Observations of V1974 Cygni (Nova Cygni 1992). The Astrophysical Journal, 631 (2). 1094-1099 doi:10.1086/432656
Hachisu, Izumi, Kato, Mariko (2003) A New Clue to the Transition Mechanism between Optical High and Low States of the Supersoft X‐Ray Source RX J0513.9−6951, Implied By the Recurrent Nova CI Aquilae 2000 Outburst Model. The Astrophysical Journal, 588 (2). 1003-1008 doi:10.1086/374303
Kato, Mariko, Hachisu, Izumi, Mikołajewska, Joanna (2013) AN X-RAY AND OPTICAL LIGHT CURVE MODEL OF THE ECLIPSING SYMBIOTIC BINARY SMC3. The Astrophysical Journal, 763 (1). 5pp. doi:10.1088/0004-637x/763/1/5
Hachisu, Izumi, Kato, Mariko (2014) THEUBVCOLOR EVOLUTION OF CLASSICAL NOVAE. I. NOVA-GIANT SEQUENCE IN THE COLOR-COLOR DIAGRAM. The Astrophysical Journal, 785 (2). 97pp. doi:10.1088/0004-637x/785/2/97
Hachisu, Izumi, Kato, Mariko, Matsumoto, Katsura (2024) A Multiwavelength Light-curve Model of the Classical Nova V339 Del: A Mechanism for the Coexistence of Dust Dip and Supersoft X-Rays. The Astrophysical Journal, 965 (1) 49 doi:10.3847/1538-4357/ad2a45
Kato, Mariko, Hachisu, Izumi (2009) MULTIPLICITY OF NOVA ENVELOPE SOLUTIONS AND OCCURRENCE OF OPTICALLY THICK WINDS. The Astrophysical Journal, 699 (2). 1293-1299 doi:10.1088/0004-637x/699/2/1293
Kato, Mariko, Hachisu, Izumi (2023) Theoretical Light-curve Models of the Symbiotic Nova CN Cha—Optical Flat Peak for 3 Yr. The Astrophysical Journal, 951 (2) 128 doi:10.3847/1538-4357/acdb4c
Kato, Mariko, Hachisu, Izumi, Cassatella, Angelo, González-Riestra, Rosario (2011) A LIGHT-CURVE MODEL OF THE SYMBIOTIC NOVA PU Vul (1979): A VERY QUIET EXPLOSION WITH LONG-LASTING FLAT PEAK. The Astrophysical Journal, 727 (2). 72pp. doi:10.1088/0004-637x/727/2/72
 
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