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Relevant bibliographies by topics / Supernova 1604

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Academic literature on the topic 'Supernova 1604'

Author: Grafiati

Published: 28 February 2023

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Journal articles on the topic "Supernova 1604"

1

de Angelis, Alessandro, and Selenia Broccio. "First Observations of SN 1604 (Kepler’s Supernova)." Universe 7, no. 11 (2021): 430. http://dx.doi.org/10.3390/universe7110430.

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A supernova close enough to the Earth is a spectacular event: it can appear as a “new star” as luminous as Venus, or even more, visible for several days. The rate of Galactic supernovae is expected to be of about one in 30 years, with a fraction visible to the naked eye; however in all the history of human civilization only seven supernovae in the Milky Way have been reported, the last two (1572 and 1604) during Galilei’s life. The supernova of 1604, today called Kepler’s Supernova, was observed by Galilei, Kepler and other astronomers in Europe, Korea, China, Arabia. Like the supernova SN1572

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Cosci, M. "Galileo’s Account of Kepler’s Supernova (SN 1604): A Copernican Assessment." Proceedings of the International Astronomical Union 14, A30 (2018): 179–80. http://dx.doi.org/10.1017/s1743921319004022.

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AbstractThe name of Kepler is inseparably associated with the supernova of 1604 (SN 1604; V843 Ophiuchi), but there are reasons why Galileo Galilei might also claim to leave his name on that phenomenon, given the assiduousness of his observations.

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Ruiz–Lapuente, Pilar, Jonay González Hernández, Hugo Tabernero, et al. "Survey for the Binary Progenitor in SN1006 and Update on SN1572." Proceedings of the International Astronomical Union 7, S281 (2011): 322–25. http://dx.doi.org/10.1017/s1743921312015293.

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AbstractWe have completed a survey down to R = 15 mag of the stars within a circle of 4 arcmin radius around the nominal center of the remnant of SN 1006, one of the three historical Type Ia supernovae (the other two being SN 1572 and SN 1604), in search of a possible surviving binary companion of the white dwarf whose explosion gave rise to the supernova. The stellar parameters (effective temperature, surface gravity, and metallicity), as well as the radial velocities of all the stars, have been measured from spectra obtained with the UVES spectrograph at the VLT, and from the former and the

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4

Green, D. W. E. "A new look at the position of the 1604 Supernova (V843 Ophiuchi)." Astronomische Nachrichten 326, no. 2 (2005): 101–11. http://dx.doi.org/10.1002/asna.200410345.

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5

Bouchet, Patrice, and John Danziger. "9500 Nights of Mid-Infrared Observations of SN 1987A: the birth of the remnant." Proceedings of the International Astronomical Union 9, S296 (2013): 9–14. http://dx.doi.org/10.1017/s1743921313009162.

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AbstractThe one-in-a-life-time event Supernova SN 1987A, the brightest supernova seen since Kepler's in 1604, has given us a unique opportunity to study the mechanics of a supernova explosion and now to witness the birth of a supernova remnant. A violent encounter is underway between the fastest-moving debris and the circumstellar ring: shocks excite “hotspots”. ATCA/ANTF, Gemini, VLT, HST, Spitzer, Chandra, and recently ALMA observations have been so far organized to help understanding the several emission mechanisms at work. In the mid-infrared SN 1987A has transformed from a SN with the bul

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6

Hughes, John P. "The Extraordinarily Rapid Expansion of the X‐Ray Remnant of Kepler’s Supernova (SN 1604)." Astrophysical Journal 527, no. 1 (1999): 298–309. http://dx.doi.org/10.1086/308082.

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7

Rotar, O. P., and K. M. Tolkunova. "EVA and SUPERNOVA concepts of vascular aging: ongoing research on damaging and protective risk factors." "Arterial’naya Gipertenziya" ("Arterial Hypertension") 26, no. 2 (2020): 133–45. http://dx.doi.org/10.18705/1607-419x-2020-26-2-133-145.

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Regarding prevention of cardiometabolic diseases, we often rely on the concepts of risk and disease, rather than the possibility of prevention. The concept of “vascular age” is developed to assess the biological state of arteries and to present cardiovascular risk in years for better understanding by the doctor and patient. Early vascular aging (EVA) syndrome has been studied for more than 10 years to determine the optimal diagnostic criteria and treatment approaches. In 2019, leading experts in the area of vascular stiffness suggested the opposite concept of supernomal vascular aging (SUPERNO

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8

Seth, A. C. "Supernova Remnant G11.2—0.3 and the ISM." Symposium - International Astronomical Union 199 (2002): 311–12. http://dx.doi.org/10.1017/s0074180900169190.

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We present 610 and 235 MHz GMRT observations of the supernova remnant (SNR) G11.2—0.3 which shows a very large roation measure gradient (ΔRM∼1600 rad m−2) across it. The GMRT observations are the first high-resolution observations of this object at low frequencies. There are differences between the structure observed at 610 and at 235 MHz only some of which can be explained by free-free absorption.

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9

Moriya, T. J., M. D. Stritzinger, F. Taddia, et al. "The Carnegie Supernova Project II." Astronomy & Astrophysics 641 (September 2020): A148. http://dx.doi.org/10.1051/0004-6361/202038118.

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We present optical and near-infrared photometry and spectroscopy of the Type IIn supernova, (SN) 2014ab, obtained by the Carnegie Supernova Project II and initiated immediately after its optical discovery. We also study public mid-infrared photometry obtained by the Wide-field Infrared Survey Explorer satellite extending from 56 days prior to the optical discovery to over 1600 days. The light curve of SN 2014ab evolves slowly, while the spectra exhibit strong emission features produced from the interaction between rapidly expanding ejecta and dense circumstellar matter. The light curve and spe

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10

Rotar, O. P., M. A. Boiarinova, K. M. Tolkunova, et al. "Vascular aging phenotypes in Russian population — biological, social, and behavioral determinants." Cardiovascular Therapy and Prevention 20, no. 5 (2021): 2970. http://dx.doi.org/10.15829/1728-8800-2021-2970.

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Aim. To assess the association of cardiovascular risk factors with various vascular aging phenotypes using the St. Petersburg population sample as part of the Epidemiology of Cardiovascular Diseases and their Risk Factors in Regions of Russian Federation (ESSE-RF) study.Material and methods. The current analysis, performed within the ESSE-RF multicenter observational study, included 1600 St. Petersburg residents. The participants filled out a questionnaire to assess risk factors. In addition, blood biochemical parameters, anthropometric characteristics, and blood pressure were evaluated. Pulse

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Books on the topic "Supernova 1604"

1

Massimo, Turatto, ed. 1604-2204: Supernovae as cosmological lighthouses : proceedings of a meeting held in Palazzo del Bo, Università degli Studi di Padova, Padua, Italy 15-19 June 2004. Astronomical Society of the Pacific, 2005.

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Book chapters on the topic "Supernova 1604"

1

Vink, Jacco. "Supernova 1604, Kepler’s Supernova, and Its Remnant." In Handbook of Supernovae. Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-20794-0_49-1.

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Vink, Jacco. "Supernova 1604, Kepler’s Supernova, and its Remnant." In Handbook of Supernovae. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-21846-5_49.

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3

Meaburn, J., M. Bryce, and A. J. Holloway. "Smoke Rings Around Supernova 1987A." In Shocks in Astrophysics. Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-009-1624-1_12.

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Raymond, J. C. "Diagnostics of Supernova Remnant Shock Waves." In Shocks in Astrophysics. Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-009-1624-1_30.

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Humphreys, Roberta M., and John C. Martin. "Eta Carinae: From 1600 to the Present." In Eta Carinae and the Supernova Impostors. Springer US, 2012. http://dx.doi.org/10.1007/978-1-4614-2275-4_1.

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6

Pedlar, A., and T. W. B. Muxlow. "Supernova Remnants in the Starburst Galaxy M82." In Shocks in Astrophysics. Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-009-1624-1_36.

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Jun, Byung-il, and Michael L. Norman. "MHD Simulations of Rayleigh-Taylor Instability in Young Supernova Remnants." In Shocks in Astrophysics. Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-009-1624-1_34.

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8

Bychkov, Vitaliy V., and Michael A. Liberman. "Self-Consistent Theory of White Dwarf Burning in Supernova IA Events." In Shocks in Astrophysics. Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-009-1624-1_37.

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9

Stephenson, F. Richard, and David A. Green. "Kepler’s SN OF AD 1604." In Historical Supernovae and their Remnants. Oxford University Press, 2002. http://dx.doi.org/10.1093/acprof:oso/9780198507666.003.0005.

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