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Orio, Marina, Balman, Soelen, della Valle, Massimo, Gallagher, Jay, Oegelman, Hakki (1996) X-Ray Emission of Nova Puppis 1991: Accretion or a Shocked Shell?. The Astrophysical Journal, 466. 410pp. doi:10.1086/177520

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Reference TypeJournal (article/letter/editorial)
TitleX-Ray Emission of Nova Puppis 1991: Accretion or a Shocked Shell?
JournalThe Astrophysical Journal
AuthorsOrio, MarinaAuthor
Balman, SoelenAuthor
della Valle, MassimoAuthor
Gallagher, JayAuthor
Oegelman, HakkiAuthor
Year1996 (July)Volume466
PublisherIOP Publishing
DOIdoi:10.1086/177520Search in ResearchGate
Generate Citation Formats
Mindat Ref. ID3339655Long-form Identifiermindat:1:5:3339655:6
GUID0
Full ReferenceOrio, Marina, Balman, Soelen, della Valle, Massimo, Gallagher, Jay, Oegelman, Hakki (1996) X-Ray Emission of Nova Puppis 1991: Accretion or a Shocked Shell?. The Astrophysical Journal, 466. 410pp. doi:10.1086/177520
Plain TextOrio, Marina, Balman, Soelen, della Valle, Massimo, Gallagher, Jay, Oegelman, Hakki (1996) X-Ray Emission of Nova Puppis 1991: Accretion or a Shocked Shell?. The Astrophysical Journal, 466. 410pp. doi:10.1086/177520
In(1996) The Astrophysical Journal Vol. 466. IOP Publishing

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Balman,, Şölen, Orio,, Marina, Ögelman, Hakkı (1995) [ITAL]ROSAT[/ITAL] Observation of the Old Classical Nova CP Puppis. The Astrophysical Journal, 449 (1). doi:10.1086/309628
Orio, Marina, Tepedelenlioglu, Emre, Starrfield, Sumner, Woodward, Charles E., Della Valle, Massimo (2005) ChandraObservations of the Recurrent Nova IM Normae. The Astrophysical Journal, 620 (2). 938-942 doi:10.1086/427207
Balman, Şölen, Ögelman, Hakki B. (1999) The First Resolved and Detected Classical Nova Shell in X-Rays: The Shell of Nova Persei 1901. The Astrophysical Journal, 518 (2). doi:10.1086/312069
Oegelman, Hakki, Finley, John P. (1993) ROSAT observations of pulsed soft X-ray emission from PSR 1055-52. The Astrophysical Journal, 413. doi:10.1086/186952
Della Valle, Massimo, Livio, Mario (1996) Are Microlensing Events Contaminated by Dwarf Nova Eruptions?. The Astrophysical Journal, 457 (2). doi:10.1086/309904
Balman, Şolen, Krautter, Joachim, Ogelman, Hakki (1998) The X‐Ray Spectral Evolution of Classical Nova V1974 Cygni 1992: A Reanalysis of theROSATData. The Astrophysical Journal, 499 (1). 395-406 doi:10.1086/305600
Ögelman, Hakki, Orio, Marina, Krautter, Joachim, Starrfield, Sumner (1993) Detection of supersoft X-ray emission from GQ Muscae nine years after a nova outburst. Nature, 361 (6410). 331-333 doi:10.1038/361331a0
Balman, Şolen (2005) ChandraObservation of the Shell of Nova Persei 1901 (GK Persei): Detection of Localized Nonthermal X‐Ray Emission from a Miniature Supernova Remnant. The Astrophysical Journal, 627 (2). 933-952 doi:10.1086/430392
Bianchini, A., Saygac, T., Orio, M., della Valle, M., Williams, R. (2012) The old nova CP Puppis: a carbon nova and asynchronous polar?. Astronomy & Astrophysics, 539. doi:10.1051/0004-6361/201117251
Mukai, K., Orio, M., Della Valle, M. (2008) Novae as a Class of Transient X‐Ray Sources. The Astrophysical Journal, 677 (2). 1248-1252 doi:10.1086/529362
Shanley, L., Ogelman, H., Gallagher, J. S., Orio, M., Krautter, J. (1995) The soft X-ray turnoff of Nova MUSCAE 1983. The Astrophysical Journal, 438. doi:10.1086/187724
 
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