Abstract
Advances in instrumentation have uncovered many new phenomena in the universe. Some have been found to repeat, either sporadically or with a more regular period. Many more are suspected to be actually repetitive; they appear as one-off events possibly due to the limitations of the period of observation. These include novae and fast radio bursts. Novae and X-ray bursts are believed to result from accretion in a binary system from a companion star onto a compact object like a white dwarf or a neutron star. Periodic oscillations are found to be associated with sporadic events like Type I X-ray bursts, though their origin is not understood. Fast radio bursts are of varied nature, indicating that origin of different classes may be different.
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Notes
- 1.
Roche lobe is the region around a star in a binary system within which orbiting material is gravitationally bound to that star.
- 2.
SN Ia occurs when the mass of the white dwarf crosses Chandrasekhar limit so that the electron degeneracy pressure can no longer sustain the star against collapse. This results in a violent explosion.
- 3.
Because of the ionised component of interstellar medium, principally due to free electrons, high-frequency components of a radio pulse arrive earlier than the low-frequency components. DM can be estimated from measurement of this delay, and can give an idea of the distance of the source.
- 4.
A neutron star with extremely strong magnetic field, of the order of \(10^9\)–\(10^{11}\)T.
References
Anupama GC (2008) One year of monitoring of the 2006 outburst in optical and low radio frequencies. In: Evans A, Bode MF, O’Brien TJ, Darnley MJ (eds) RS Ophiuchi (2006) the recurrent nova phenomenon, ASP conference series 401. ASP, San Francisco, p 31
Mukai K (2014) Recurrent novae - a review. Acta Polytechnica CTU Proc 2:246
Darnley MJ (2019) Accrete, accrete, accrete ... bang! (and repeat): the remarkable recurrent novae. In: Proceedings of the golden age of cataclysmic variables and related objects V, proceedings of science, vol 368
Schaefer BE (2023) The recurrent nova T CrB had prior eruptions observed near December 1787 and October 1217 AD. J Hist Astron 54:436
Evans A, Banerjee DPK, Woodward CE, Geballe TR, Gehrz RD, Page KL, Starrfield S (2023) Infrared spectroscopy of the 2022 eruption of the recurrent nova U Sco. MNRAS 522:4841
Clark GW, Jernigan JG, Bradt H, Canizares C, Lewin WHG, Li FK, Mayer W, McClintock J, Schnopper H (1976) Recurrent brief X-ray bursts from the globular cluster NGC 6624. ApJ 207:L 015
Grindlay J, Gursky H, Schnopper H, Parsignault DR, Heise J, Brinkman AC, Schrijver J (1976) Discovery of intense X-ray bursts from the globular cluster NGC 6624. ApJ 205:L 127
Galloway DK, Keek L (2021) Thermonuclear X-ray bursts. In: Belloni TM, Méndez M, Zhang C, (eds) Timing neutron stars: pulsations, oscillations and explosions. Astrophysics and space science library, vol 461. Springer, Berlin, Heidelberg
Galloway DK, in ’t Zand J, Chenevez J, Wörpel H, Keek L, Ootes L, Watts AL, Gisler L, Sanchez-Fernandez C, Kuulkers E (2020) The Multi-INstrument Burst ARchive (MINBAR. ApJS 249:32
Lahiri C, Gangopadhyay G (2012) Endpoint of rp process using relativistic mean field approach and a new mass formula. Int J Modern Phys E 21:1250074
Strohmayer TE, Zhang W, Swank JH, Smale A, Titarchuk L (1996) Millisecond X-Ray variability from an accreting neutron star system. ApJ 469:L9
Chakrabarty D, Morgan EH, Muno MP, Galloway DK, Wijnands R, ven der Klis M, Markwardt CB (2003) Nuclear-powered millisecond pulsars and the maximum spin frequency of neutron stars. Nature 424:42
Watts AL (2012) Thermonuclear burst oscilations. Ann Rev Astron Astrophys 50:609
Lewin WHG, Doty J, Clark GW, Rappaport SA, Bradt HVD, Doxsey R, Hearn DR, Hoffman JA, Jernigan JG, Li FK, Mayer W, McClintock J, Primini F, Richardson J (1976) The discovery of rapidly repetitive X-ray bursts from a new source in Scorpius. ApJ 207:L95
van der Eijnden JJ, Bagnoli T, Degenaar N, Lohfink AM, Parker ML, in ’t Zand JJM, Fabian AC (2017) A strongly truncated inner accretion disk in the Rapid Burster. MNRAS 466:L98
Spruit HC, Tamm RE (1993) An instability associated with a magnetosphere-disk interaction. ApJ 402:593; D’Angelo CR, Spruit HC (2010) Episodic accretion on to strongly magnetic stars. MNRAS 406:1208
Degenaar N, Miller JM, Harrison FA, Kennea JA, Kouveliotou C, Younes G (2014) High-resolution X-Ray spectroscopy of the bursting pulsar GRO J1744–28. ApJL 796:L9
Lorimer DR, Bailes M, Mclaughin MA, Narkevic DJ, Crawford F (2007) A bright millisecond radio burst of extragalactic origin. Science 318:777
Scholz P, (on behallf of Chime/FRB) Collaboration (2020) A bright millisecond-timescale radio burst from the direction of the Galactic magnetar SGR 1935+2154. Astron Telegr, ATel # 13681
Petroff E, Hessels JWT, Lorimer DR (2019) Fast radio bursts. Astron Astrophys Rev 27:4
Bannister KW et al (2017) The detection of an extremely bright fast radio burst in a phased array feed survey. ApJL 841:L 12
Spitler LG et al (2014) Fast radio burst discovered in the arecibo pulsar ALFA survey. ApJ 790:101
Spitler LG et al (2016) A repeating fast radio burst. Nature 531:202
Chatterjee S et al (2017) A direct localisation of a fast radio burst and its host. Nature 541:58
Marcote B et al (2017) The repeating fast radio burst FRB 121102 as seen on milliarcsecond angular scales. ApJL 834:L8
The CHIME/FRB Collaboration (2021) The first CHIME/FRB fast radio burst catalog. ApJS 257:59
The CHIME/FRB Collaboration (2020) Periodic activity from a fast radio burst source. Nature 582:351
Marcote B et al (2020) A repeating fast radio burst source localised to a nearby spiral galaxy. Nature 577:190
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Gangopadhyay, G., Kundu, A. (2024). Strange Rhythms, Strange Objects. In: Rhythm in the Sky. Studies in Rhythm Engineering. Springer, Singapore. https://doi.org/10.1007/978-981-97-2588-5_8
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