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- usando fotometría CCD de Banda V con un reflector de 60 cm, y observaron superhumps (oscilaciones periódicas superpuestas) de magnitud 0.1, reclasificando…2 kB (220 palabras) - 21:10 7 feb 2023
- cataclysmic variable TT Arietis. QPO behaviour coming back from positive superhumps». Astronomy and Astrophysics 496 (3). pp. 765-775. Datos: Q4050619…5 kB (508 palabras) - 17:16 23 ene 2024
Resultados de la Wikipedia en inglés.
- precession of the disk causes negative superhumps, with periods slightly less than the orbital period. Superhumps can occur in dwarf nova systems in which…3 kB (399 palabras) - 14:14 24 oct 2022
- Cataclysmic variable star (sección Superhumps)In astronomy, cataclysmic variable stars (CVs) are stars which irregularly increase in brightness by a large factor, then drop back down to a quiescent…11 kB (961 palabras) - 02:26 6 nov 2023
- large outbursts, some dwarf novae show periodic brightening known as “superhumps”. They are caused by deformations of the accretion disk when its rotation…7 kB (701 palabras) - 15:46 17 ene 2024
- outbursts, known as superhumps. The normal outbursts result in an increase in brightness lasting around a day every 37 days, while the superhumps last 5–20 days…37 kB (4058 palabras) - 18:04 25 abr 2024
- supereruptions. The former are smooth, while the latter exhibit short "superhumps" of heightened activity. One of the brightest dwarf novae in the sky,…29 kB (3095 palabras) - 21:09 30 abr 2024
- supereruptions. The former are smooth, while the latter exhibit short "superhumps" of heightened activity. The distance of the system has been assumed at…7 kB (711 palabras) - 00:07 11 sep 2023
- supereruptions. The former are smooth, while the latter exhibit short "superhumps" of heightened activity. The white dwarf sucks matter from the other star…2 kB (233 palabras) - 12:34 14 may 2023
- brightness lasting around a day every 37 days. Brighter outbursts, known as superhumps, last 5-20 days and take place every 194 days. The properties of TU Mensae…4 kB (359 palabras) - 13:35 24 feb 2023
- Kazuyuki; Ono, Rikako (2013-02-01). "Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. IV. The Fourth Year (2011-2012)". Publications…6 kB (559 palabras) - 23:15 30 may 2024
- until dawn." Superhumps in Cataclysmic Binaries (2005). A paper co-authored by McCormick that described the search for positive superhumps in cataclysmic…18 kB (1594 palabras) - 19:50 19 feb 2024
- positive superhump was observed in 2000 - 2003, while 80.376 min negative superhumps were seen in 2013 and 2014. This is the first time negative superhumps have…13 kB (899 palabras) - 15:50 5 ene 2024
- Skillman, David R.; Patterson, Joseph; Thorstensen, John R. (1995). "Superhumps in Cataclysmic Binaries. IV. MV Lyrae". Publications of the Astronomical…69 kB (7587 palabras) - 11:51 7 jun 2024
- Boneva, Daniela; et al. (November 2022), "Recent observations of humps and superhumps and an estimation of outburst parameters of the AM CVn star CR Boo", Astrophysics…14 kB (978 palabras) - 09:16 13 ago 2023
- supereruptions. The former are smooth, while the latter exhibit short "superhumps" of heightened activity and last 2.6% longer. SX Leonis Minoris has been…4 kB (420 palabras) - 18:43 26 abr 2024
- Monitoring of the Microquasar GRS 1915+105: Detection of Orbital and Superhump Signatures". The Astrophysical Journal. 657 (1): 409–414. arXiv:astro-ph/0610480…9 kB (804 palabras) - 15:13 30 abr 2024
- outbursts cycle (they were observed only in 1979, 1994 and 2004) and superhumps can be observed with a short periodic modulation. It was observed also…5 kB (397 palabras) - 18:06 23 feb 2023
- ; Bianchini, A.; Bonibaker, J.; della Valle, M.; Vio, R. (1996), "The superhump phenomenon in GRS 1716-249 (=X-Ray Nova Ophiuchi 1993)", Astronomy and…40 kB (4015 palabras) - 23:43 18 may 2024
- classified as a slow nova and its light curve exhibits positive superhumps, meaning superhumps with a period a few percent (8.6% in this case) longer than…8 kB (806 palabras) - 11:40 10 sep 2023
- ; Lipkin, Y.; Retter, A.; Leibowitz, E. (June 1998). "Observation of Superhumps in SS UMi". Information Bulletin on Variable Stars. 4602: 1. Bibcode:1998IBVS…3 kB (254 palabras) - 11:51 14 may 2023
- the system is similar to ER Ursae Majoris, showing superoutbursts and superhumps. This indicates that RZ LMi is a SU Ursae Majoris-type dwarf novae belonging…13 kB (971 palabras) - 00:13 11 sep 2023
- between superoutbursts) is very short at around 43 days. Large amplitude superhumps were found to occur near the start of a superoutburst, with a brightness…13 kB (1037 palabras) - 23:39 10 sep 2023