Relevant bibliographies by topics / Compact object (Astronomy)

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers

Academic literature on the topic 'Compact object (Astronomy)'

Author: Grafiati
Published: 4 June 2021
Last updated: 12 February 2022

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Journal articles on the topic "Compact object (Astronomy)"

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van der Sluys, M. V., C. Röver, A. Stroeer, V. Raymond, I. Mandel, N. Christensen, V. Kalogera, R. Meyer, and A. Vecchio. "Gravitational-Wave Astronomy with Inspiral Signals of Spinning Compact-Object Binaries." Astrophysical Journal 688, no. 2 (October 23, 2008): L61—L64. http://dx.doi.org/10.1086/595279.

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Pfeiffer, Harald P. "Numerical simulations of compact object binaries." Classical and Quantum Gravity 29, no. 12 (June 1, 2012): 124004. http://dx.doi.org/10.1088/0264-9381/29/12/124004.

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Kalogera, Vassiliki. "Binary compact object inspiral: Detection expectations." Pramana 63, no. 4 (October 2004): 673–83. http://dx.doi.org/10.1007/bf02705191.

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Kavic, Michael, Steven L. Liebling, Matthew Lippert, and John H. Simonetti. "Accessing the axion via compact object binaries." Journal of Cosmology and Astroparticle Physics 2020, no. 08 (August 4, 2020): 005. http://dx.doi.org/10.1088/1475-7516/2020/08/005.

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Breivik, Katelyn, Sourav Chatterjee, and Jeff J. Andrews. "Constraining Compact Object Formation with 2M0521." Astrophysical Journal 878, no. 1 (June 5, 2019): L4. http://dx.doi.org/10.3847/2041-8213/ab21d3.

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Li, Xinyu, Philip Chang, Yuri Levin, Christopher D. Matzner, and Philip J. Armitage. "Simulation of a compact object with outflows moving through a gaseous background." Monthly Notices of the Royal Astronomical Society 494, no. 2 (April 9, 2020): 2327–36. http://dx.doi.org/10.1093/mnras/staa900.

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ABSTRACT A compact object moving relative to surrounding gas accretes material and perturbs the density of gas in its vicinity. In the classical picture of Bondi–Hoyle–Lyttleton accretion, the perturbation takes the form of an overdense wake behind the object, which exerts a dynamical friction drag. We use hydrodynamic simulations to investigate how the accretion rate and strength of dynamical friction are modified by the presence of outflow from the compact object. We show that the destruction of the wake by an outflow reduces dynamical friction, and reverses its sign when the outflow is strong enough, in good quantitative agreement with analytic calculations. For a strong isotropic outflow, the outcome on scales that we have simulated is a negative dynamical friction, i.e. net acceleration. For jet-like outflows driven by reprocessed accretion, both the rate of accretion and the magnitude of dynamical friction drop for more powerful jets. The accretion rate is strongly intermittent when the jet points to the same direction as the motion of the compact object. The dynamical effects of outflows may be important for the evolution of compact objects during the common envelope phase of binary systems, and for accreting compact objects and massive stars encountering active galactic nucleus discs.
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Wiktorowicz, Grzegorz, Matthew Middleton, Norman Khan, Adam Ingram, Poshak Gandhi, and Hugh Dickinson. "Predicting the self-lensing population in optical surveys." Monthly Notices of the Royal Astronomical Society 507, no. 1 (July 29, 2021): 374–84. http://dx.doi.org/10.1093/mnras/stab2135.

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ABSTRACT The vast majority of binaries containing a compact object and a regular star spend most of their time in a quiescent state where no strong interactions occur between components. Detection of these binaries is extremely challenging and only few candidates have been detected through optical spectroscopy. Self-lensing represents a new means of detecting compact objects in binaries, where gravitational lensing of the light from the visible component by the compact object produces periodic optical flares. Here we show that current and planned large-area optical surveys can detect a significant number (∼100–10 000s) of these self-lensing binaries and provide insights into the properties of the compact lenses. We show that many of the predicted population of observable self-lensing binaries will be observed with multiple self-lensing flares; this both improves the chances of detection and also immediately distinguishes them from chance-alignment micro-lensing events. Through self-lensing we can investigate long – but previously hidden – stages of binary evolution and consequently provide new constraints on evolutionary models that impact the number and nature of double compact object mergers.
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Tremblay, S. E., G. B. Taylor, J. F. Helmboldt, C. D. Fassnacht, and T. J. Pearson. "A Shrinking Compact Symmetric Object: J11584+2450?" Astrophysical Journal 684, no. 1 (September 2008): 153–59. http://dx.doi.org/10.1086/590377.

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Fryer, Chris L. "Compact object formation and the supernova explosion engine." Classical and Quantum Gravity 30, no. 24 (November 29, 2013): 244002. http://dx.doi.org/10.1088/0264-9381/30/24/244002.

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Tanaka, Y. "Observations of Compact X-Ray Sources." International Astronomical Union Colloquium 89 (1986): 198–221. http://dx.doi.org/10.1017/s0252921100086097.

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This paper reviews the present status of observations of compact X-ray sources with emphasis on the aspects related to radiation hydrodynamics, based on the recent observational results, in particular those from the Japanese X-ray astronomy satellite Tenma. The main feature of Tenma is a large-area gas scintillation proportional counters (GSPC) with energy resolution twice that of ordinary proportional counters, which can yield information on energy spectrum superior in quality to previous results. We shall deal here only with those galactic X-ray sources in which the compact object is a neutron star or possibly a black hole, and exclude white dwarf sources.There exist more than one hundred bright X-ray sources in our galaxy in the luminosity range 1036−1038 ergs/sec. They are most probably binaries involving a neutron star or, in some cases, possibly a black hole. The high luminosities of these sources are explained in terms of the large gravitaional energy release by matter accreting from the companion star to the compact object.
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Dissertations / Theses on the topic "Compact object (Astronomy)"

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van, Spaandonk Lieke. "Exploring new emission line diagnostics for accreting compact objects." Thesis, University of Warwick, 2011. http://wrap.warwick.ac.uk/55659/.

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Theory predicts that a large fraction of CVs should have passed through the minimum period. The Sloan Digital Sky Survey (sdss) sample is finally unearthing these systems in large numbers. But due to their faint donor stars, the orbital period is often the only measurable system parameter for most CVs. The indirect measurable of the superhump period, and hence superhump excess, could potentially provide an indication of the mass ratio of the systems via the empirical relation between the two observables. While this relation is potentially very useful for the determination of mass ratios, the large scatter in the calibrators, especially at the low mass ratio end, prohibits a direct conversion between easy to measure light curve variability and the much sought after mass ratio. To place a short period CV firmly on the evolutionary track (e.g pre- or post bounce systems), more direct methods to determine the mass ratio are required, as well as a better calibration and validation of the relation between the superhump excess and mass ratio. We can achieve this, by constraining the mass ratios of short period CVs using dynamical constraints on the radial velocities of the binary components. The radial velocity of the WD (K1) is only occasionally directly measurable as the WD features are typically swamped by the strong disc features. As the disc is centred on the WD, measuring the disc radial velocity can give an indication of the WD radial velocity, but these measures tend to be biased by hotspots and other asymmetries in the disc. Measuring the radial velocity of the donor star (K2) is less straightforward and normally performed by either measuring the radial velocity of the donor absorption lines for earlier type donor stars, or via emission lines associated with the donor star, if irradiated by the disc and WD. The first method fails in short period CVs as the faint features from the late type donors in these systems are concealed in the accretion and WD dominated optical spectrum, even at very low mass loss rates. The second method comes with tight timing constraints as the irradiated donor is generally only visible on top of the double peaked disc emission shortly after outburst and data needs to be obtained via target of opportunity programs. In this thesis, we present a spectroscopic survey of short periods CVs and explore new techniques in addition to the traditional methods for the determination of the radial velocity components. We combine these new methods with the exploitation of the more `exotic' Ca ii triplet lines in the I-band in addition to the commonly used Balmer lines. We will show that, while it suffers from some of the same systematics as the Balmer lines, we can measure K1 better in Ca ii than in Balmer, especially when exploiting Doppler maps for these measures. More importantly for many systems, donor emission is visible in the Ca ii lines, which provides us with measures for the radial velocity amplitude of this feature (Kem). These, combined with K-correction models, yield a good measure of K2. We find that the determination of Kem is easy in Doppler maps, and that the K-correction, via irradiation methods, is fairly solid. We use these values to dynamically constrain the mass ratios for 13 CVs, including several eclipsing systems to test the validity of our method. The survey includes well known systems such as GW Lib, WZ Sge, OY Car and IP Peg.
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Huerta, Escudero Eliu Antonio. "Source modelling of extreme and intermediate mass ratio inspirals." Thesis, University of Cambridge, 2011. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.609770.

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Fang, Xiao. "Perturbation Theories in Astrophysics: From Large-Scale Structure To Compact Objects." The Ohio State University, 2018. http://rave.ohiolink.edu/etdc/view?acc_num=osu1531217962535791.

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Völkel, Sebastian [Verfasser], and Kostas [Akademischer Betreuer] Kokkotas. "On the Gravitational Wave Spectrum of Compact Relativistic Objects / Sebastian Völkel ; Betreuer: Kostas Kokkotas." Tübingen : Universitätsbibliothek Tübingen, 2020. http://d-nb.info/1212024931/34.

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Efremov, Pavel [Verfasser], Volker [Akademischer Betreuer] Perlick, Volker [Gutachter] Perlick, and Domenico [Gutachter] Giulini. "Relativistic accretion onto compact objects / Pavel Efremov ; Gutachter: Volker Perlick, Domenico Giulini ; Betreuer: Volker Perlick." Bremen : Staats- und Universitätsbibliothek Bremen, 2018. http://d-nb.info/1164151983/34.

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Valente, Ema Filipa dos Santos. "A simple model of exotic compact objects : interaction with a scalar field." Master's thesis, Universidade de Aveiro, 2017. http://hdl.handle.net/10773/23655.

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Mestrado em Física
Modelos de objetos compactos exóticos (OCEs) foram propostos nas últimas décadas como alternativas aos buracos negros. Esses modelos visam reproduzir a fenomenologia que caracteriza os (candidatos a) buracos negros observados. No entanto, para superar os problemas associados ao horizonte de eventos (e à consequente singularidade de curvatura, de acordo com o teorema de Penrose), estes OCEs não possuem horizonte de eventos. Nesta dissertação, exploramos um modelo simples de um OCE, descrito pela métrica de Kerr-Newman no exterior de uma superfície com condições de fronteira reflectivas, localizada fora do horizonte de eventos de Kerr-Newman. Nesta geometria, estudamos OCEs que podem estar em equilíbrio com con figurações estáticas de um campo escalar. Consideramos um campo escalar sem massa, tanto no caso eletricamente não carregado como no caso carregado, e obtemos, através de métodos analíticos, um conjunto discreto de raios críticos da superfície do OCE que podem suportar con figurações estáticas não triviais do campo escalar. Dentro deste conjunto discreto, o OCE com maior raio crítico separa os OCEs estáveis e instáveis relativamente à instabilidade superradiante, induzida por um campo escalar. O conjunto discreto de raios críticos da superfície do OCE foi construído para os três regimes diferentes da métrica de Kerr-Newman: regime sub-extremo, regime extremo e regime super-extremo. Estes espectros de ressonância dependem dos parâmetros físicos {a, Q, q, l,m }
Models of exotic compact objects (ECOs) have been proposed in the past decades as alternatives to black holes. These models aim at reproducing the phenomenology that characterises the observed black hole (candidates). However, to overcome the problems associated to the event horizon (and the consequent curvature singularity, following from Penrose's singularity theorem), these ECOs do not possess an event horizon. In this thesis, we explore a simple ECO model, described by the Kerr-Newman metric in the exterior of a surface wherein re ective boundary conditions are imposed, placed outside the event horizon of the Kerr-Newman geometry. We then study, on this geometry, ECOs that may be in equilibrium with static scalar eld con- gurations. We consider both electrically charged and uncharged massless scalar elds, and, using analytical methods, we obtain a discrete set of critical ECO surface radii that can support static scalar eld con gurations. Within this discrete set, the ECO with the largest critical surface radius separates stable and unstable Kerr-Newman-type ECOs against the superradiant instability induced by a scalar eld. The discrete set of ECO critical surface radii was constructed for three di erent regimes of the Kerr-Newman metric: sub-extremal regime, extremal regime and super-extremal regime. These resonance spectra are dependent on the physical parameters {a,Q,q,l,m}
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Nativi, Lorenzo. "Jet-wind interaction in neutron star mergers." Licentiate thesis, Stockholms universitet, Institutionen för astronomi, 2020. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-189245.

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Besides being sources of gravitational waves, there has been evidence that neutron starmergers release neutron-rich material suitable for the production of heavy r-process nuclei.The radioactive decay of these freshly synthesised elements powers a rapidly evolvingthermal transient, the “macronova” (also known as “kilonova”). Its spectral propertiesstrongly depend on the ejecta composition, since neutron rich material synthesises heavyr-process elements that can efficiently trap radiation inside the ejecta producing a longlasting signal peaking in the red part of the spectrum. The first detection of a binaryneutron star merger was also accompanied by the evidence of a relativistic jet. Despitebeing ascertained the presence of these two dynamical components, neutron-rich ejectaand ultra-relativistic jet, the observational consequences of the interplay between the twois still unclear. In the paper we investigate such interaction through dedicated specialrelativistic hydrodynamic simulations, starting from a realistic environment obtained byprevious works. Light curves are then constructed up to the time scale of days by postprocessing the hydrodynamic results adopting proper radiative transfer. I show thatjet propagation within such environment can significantly affect the observation of theradioactive transient. A relativistic outflow can in fact “punch-away” a fraction of highopacity material before the brightening of the macronova, resulting in the transient beingbrighter and bluer for on-axis observers in the first few days. In this way the jet impactsboth time scale and luminosity of the macronova peak, that are the two main observablesallowing the estimate of the ejecta properties.
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Rosado, González Pablo Antonio [Verfasser]. "Gravitational wave background from compact objects and a new search for supermassive black hole binaries / Pablo Antonio Rosado González." Hannover : Technische Informationsbibliothek und Universitätsbibliothek Hannover (TIB), 2013. http://d-nb.info/1047352435/34.

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Hanke, Manfred [Verfasser], and Jörn [Akademischer Betreuer] Wilms. "Probing the Environment of Accreting Compact Objects = Untersuchung der Umgebung von akkretierenden kompakten Objekten / Manfred Hanke. Betreuer: Jörn Wilms." Erlangen : Universitätsbibliothek der Universität Erlangen-Nürnberg, 2011. http://d-nb.info/1015474926/34.

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Waisberg, Idel Reis [Verfasser], and Reinhard [Akademischer Betreuer] Genzel. "Optical interferometry of compact objects : testing general relativity and the extremes of accretion / Idel Reis Waisberg ; Betreuer: Reinhard Genzel." München : Universitätsbibliothek der Ludwig-Maximilians-Universität, 2019. http://d-nb.info/1193924197/34.

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Books on the topic "Compact object (Astronomy)"

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Herstmonceux, Conference (33rd 1992 Cambridge England). The nature of compact objects in active galactic nuclei: Proceedings of the 33rd Herstmonceux conference, held in Cambridge, July 6-22 [i.e. 16-22], 1992. Cambridge: Cambridge University Press, 1994.

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Ye-Fei, Yuan, Li Xiang-Dong, and Lai Dong, eds. Astrophysics of compact objects: International Conference on Astrophysics of Compact Objects, Huangshan City, China, 1-7 July 2007. Melville, N.Y: American Institute of Physics, 2008.

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Compact objects in astrophysics: White dwarfs, neutron stars, and black holes. Berlin: Springer, 2007.

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Physics of relativistic objects in compact binaries: From birth to coalescence. Dordrecht: Springer, 2009.

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Symposium, International Astronomical Union. Feeding compact objects: Accretion on all scales : proceedings of the 290th Symposium of the International Astronomical Union held in Beijing, China, August 20-24, 2012. Cambridge, United Kingdom: New York, USA, 2013.

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MHD flows in compact astrophysical objects: Accretion, winds and jets. Heidelberg: Springer, 2010.

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David, Blaschke, Sedrakian David, and NATO Public Diplomacy Division, eds. Superdense QCD matter and compact stars. Dordrecht: Springer., 2006.

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Symposium, International Astronomical Union. Compact stars in binaries: Proceedings of the 165th symposium of the International Astronomical Union, held in the Hague, The Netherlands, August 15-19, 1994. Dordrecht [The Netherlands]: Kluwer Academic Publishers, 1996.

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Mason, K. O. The Physics of Accretion onto Compact Objects: Proceedings of a Workshop Held in Tenerife, Spain April 21-25, 1986. Berlin, Heidelberg: Springer Berlin Heidelberg, 1986.

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Glendenning, Norman K. Compact stars: Nuclear physics, particle physics, and general relativity. New York: Springer, 1997.

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Book chapters on the topic "Compact object (Astronomy)"

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Raychaudhuri, A. K., S. Banerji, and A. Banerjee. "Accretion onto Compact Objects." In Astronomy and Astrophysics Library, 192–205. New York, NY: Springer New York, 1992. http://dx.doi.org/10.1007/978-1-4612-2754-0_15.

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Raychaudhuri, A. K., S. Banerji, and A. Banerjee. "Stellar Evolution, Supernovae, and Compact Objects." In Astronomy and Astrophysics Library, 138–43. New York, NY: Springer New York, 1992. http://dx.doi.org/10.1007/978-1-4612-2754-0_11.

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Habing, Harm J. "1995–2015: What is left: Compact Objects." In Historical & Cultural Astronomy, 407–32. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-99082-8_13.

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van der Klis, M. "Quantifying Rapid Variability in Accreting Compact Objects." In Statistical Challenges in Modern Astronomy II, 321–31. New York, NY: Springer New York, 1997. http://dx.doi.org/10.1007/978-1-4612-1968-2_18.

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Moffat, John W. "Gravitation and Black Holes." In The Shadow of the Black Hole, 11–23. Oxford University Press, 2020. http://dx.doi.org/10.1093/oso/9780190650728.003.0001.

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Einstein’s theory of general relativity introduced the concept of black holes to physics and astronomy. But, eminent physicists such as Einstein and Eddington did not believe in the existence of black holes. Schwarzschild solved Einstein’s equations and disclosed a possible dark compact object with an event horizon. This is a membrane in spacetime surrounding the object, from which nothing can escape, not even light. The chapter describes the contributions of Chandrasekhar, Kruskal, Wheeler, Oppenheimer, Landau, Kerr, and others to help promote black holes in the physics and astronomy communities. It details ideas about the origins of black holes and the conundrums they still present, such as the singularities (infinitely dense matter) associated with them.
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Andersson, Nils. "The stellar graveyard." In Gravitational-Wave Astronomy, 177–206. Oxford University Press, 2019. http://dx.doi.org/10.1093/oso/9780198568032.003.0009.

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This chapter introduces the different classes of compact objects—white dwarfs, neutron stars, and black holes—that are relevant for gravitational-wave astronomy. The ideas are placed in the context of developing an understanding of the likely endpoint(s) of stellar evolution. Key ideas like Fermi gases and the Chandrasekhar mass are discussed, as is the emergence of general relativity as a cornerstone of astrophysics in the 1950s. Issues associated with different formation channels for, in particular, black holes are considered. The chapter ends with a discussion of the supermassive black holes that are found at the centre of galaxies.
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Conference papers on the topic "Compact object (Astronomy)"

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Poggiani, Rosa. "Gravitational wave astronomy with compact binary mergers." In The Golden Age of Cataclysmic Variables and Related Objects V. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.368.0052.

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Pandey, Shashi Bhushan. "The 3.6m Devasthal optical telescope and time domain astronomy." In SN 1987A, Quark Phase Transition in Compact Objects and Multimessenger Astronomy. Институт ядерных исследования Российской академии наук, 2018. http://dx.doi.org/10.26119/sao.2020.1.52328.

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Jeffery, Elizabeth. "Late-type Compact Objects." In Frank N. Bash Symposium 2011: New Horizons in Astronomy. Trieste, Italy: Sissa Medialab, 2012. http://dx.doi.org/10.22323/1.149.0005.

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Baryshev, Yu V., and S. A. Oschepkov. "Gravitation theory in multimessenger astronomy II: crucial observational tests based on GW and optical observations." In SN 1987A, Quark Phase Transition in Compact Objects and Multimessenger Astronomy. Институт ядерных исследования Российской академии наук, 2018. http://dx.doi.org/10.26119/sao.2020.1.52285.

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Rudenko, V. N. "Current status of GW experiment and multi-messenger astronomy." In Quark Phase Transition in Compact Objects and Multimessenger Astronomy: Neutrino Signals, Supernovae and Gamma-Ray Bursts. СНЕГ, 2016. http://dx.doi.org/10.26119/sao.2020.1.51258.

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Baryshev, Yu V., and S. A. Oschepkov. "Gravitation theory in multi-messenger astronomy I: comparison of geometrical and field approaches to the physics of gravitational interaction." In SN 1987A, Quark Phase Transition in Compact Objects and Multimessenger Astronomy. Институт ядерных исследования Российской академии наук, 2018. http://dx.doi.org/10.26119/sao.2020.1.52283.

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Beskin, G. M., S. V. Karpov, V. L. Plokhotnichenko, Yu A. Shibanov, D. A. Zyuzin, A. F. Kholtygin, V. V. Sokolov, and Yu V. Baryshev. "High time resolution multi-band photo-polarimetric observations of the binary millisecond redback pulsar J1023+0038 with the BTA." In SN 1987A, Quark Phase Transition in Compact Objects and Multimessenger Astronomy. Институт ядерных исследования Российской академии наук, 2018. http://dx.doi.org/10.26119/sao.2020.1.52286.

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Bezrukov, L. B., A. S. Kurlovich, B. K. Lubsandorzhiev, A. K. Mezhokh, V. P. Morgalyuk, V. V. Sinev, and V. P. Zavarzina. "New vision of problem of Geoneutrinos and Earth heat fluxes." In SN 1987A, Quark Phase Transition in Compact Objects and Multimessenger Astronomy. Институт ядерных исследования Российской академии наук, 2018. http://dx.doi.org/10.26119/sao.2020.1.52288.

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Boliev, M. M., A. V. Butkevich, I. M. Dzaparova, M. M. Kochkarov, R. V. Novoseltseva, V. B. Petkov, P. S. Striganov, V. I. Volchenko, and A. F. Yanin. "EARCH FOR ASTROPHYSICAL NEUTRINO SOURCES AT THE BAKSAN UNDERGROUND SCINTILLATION TELESCOPE." In SN 1987A, Quark Phase Transition in Compact Objects and Multimessenger Astronomy. Институт ядерных исследования Российской академии наук, 2018. http://dx.doi.org/10.26119/sao.2020.1.52297.

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Castro-Tirado, Alberto J., Vladimir V. Sokolov, and Sergey S. Guziy. "Gamma-ray bursts: Historical afterglows and early-time observations." In SN 1987A, Quark Phase Transition in Compact Objects and Multimessenger Astronomy. Институт ядерных исследования Российской академии наук, 2018. http://dx.doi.org/10.26119/sao.2020.1.52298.

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