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8-04-2011 Sparavigna, A.C.; Marazzato, R. (10 de mayo de 2010). Observing stellar bow shocks. Bibcode:2010arXiv1005.1527S. arXiv:1005.1527. Paschmann, G.; Schwartz…19 kB (2486 palabras) - 03:03 23 jun 2024
Resultados de la Wikipedia en inglés.
- astrophysics, bow shocks are shock waves in regions where the conditions of density and pressure change dramatically due to blowing stellar wind. Bow shock occurs…18 kB (2052 palabras) - 12:29 23 ago 2024
- Magnetosphere (sección Bow shock)S2CID 122318569. Sparavigna, A.C.; Marazzato, R. (10 May 2010). "Observing stellar bow shocks". arXiv:1005.1527 [physics.space-ph]. Pokhotelov, D.; von Alfthan…21 kB (2382 palabras) - 04:06 12 oct 2024
- ; Stevens, I. R.; Isequilla, N. L. (2012). "E-BOSS: An Extensive stellar BOw Shock Survey. I. Methods and first catalogue". Astronomy & Astrophysics…40 kB (4852 palabras) - 14:11 25 oct 2024
- commencements. The bow shocks formed around planets in stellar winds, and sometimes around stars themselves. Supernova remnants driving a shock through the interstellar…4 kB (450 palabras) - 16:43 10 dic 2023
- Heliosphere (redirección desde Termination shock)Our Solar System". Live Science. Retrieved 12 October 2018. "No Shocks for This Bow: IBEX Says We're Wrong". 14 May 2012. Archived from the original…63 kB (6605 palabras) - 10:19 19 oct 2024
- Orion Nebula (sección Stellar wind and effects)become shocks when they encounter relatively stationary gases. Warped shocks appear bow-like to an observer. They are produced when a jet-driven shock encounters…45 kB (4810 palabras) - 20:25 23 sep 2024
- stellar emission lines of doubly ionized magnesium and singly ionized helium. HD 161056 is a runaway star and a candidate for producing a bow shock observable…13 kB (1243 palabras) - 18:49 6 nov 2024
- light-years). It is notable for its highly collimated jet and very symmetric bow shocks. A bipolar jet from the young star is ramming into surrounding medium…3 kB (248 palabras) - 06:37 11 dic 2023
- A stellar wind is a flow of gas ejected from the upper atmosphere of a star. It is distinguished from the bipolar outflows characteristic of young stars…5 kB (592 palabras) - 03:27 3 ago 2023
- Betelgeuse (sección Supersonic bow shock)Hertzsprung–Russell diagram, with accompanying rapid changes to their stellar winds and bow shocks." Moreover, if future research bears out this hypothesis, Betelgeuse…174 kB (18 522 palabras) - 07:28 1 nov 2024
- Zeta Ophiuchi (sección Bow shock)the Earth. It is surrounded by the Sh2-27 "Cobold" nebula, the star's bow shock as it ploughs through dense dust clouds near the Rho Ophiuchi cloud complex…21 kB (1895 palabras) - 05:52 26 oct 2024
- It also contains a mostly unipolar molecular outflow, and two large bow shocks on opposite sides of the source star. The overall size of the complex…15 kB (1714 palabras) - 18:42 19 mar 2024
- In astronomy, stellar kinematics is the observational study or measurement of the kinematics or motions of stars through space. Stellar kinematics encompasses…60 kB (7016 palabras) - 21:20 1 oct 2024
- bubbles and 599 candidate IR bow shock candidates. With a subset of highly reliable subset of 1394 IR bubbles and 453 bow shocks. The lower number of bubbles…9 kB (1016 palabras) - 00:56 29 sep 2024
- stars produce shocks in the ambient medium on encounter, resulting in generation of visible light. With the discovery of the first proto-stellar jet in HH…36 kB (4004 palabras) - 16:10 8 nov 2024
- as this with a stellar wind that is moving at supersonic velocity through the interstellar medium have their wind confined by a bow shock due to ram pressure…14 kB (1325 palabras) - 17:38 26 oct 2024
- Radiative zone (redirección desde Eddington stellar model)Introduction to Stellar Astrophysics (1st ed.). John Wiley and Sons. p. 168. ISBN 978-1-119-96497-1. Pols, Onno Rudolf (2011). Stellar Structure and Evolution…11 kB (1732 palabras) - 00:52 27 oct 2024
- ; Stevens, I. R.; Isequilla, N. L. (2012). "E-BOSS: An Extensive stellar BOw Shock Survey. I. Methods and first catalogue". Astronomy & Astrophysics…11 kB (865 palabras) - 12:04 2 ago 2024
- and shock waves. Bow shocks formed in solar winds are a direct result of transonic winds from a star. It had been long thought that a bow shock was present…14 kB (1665 palabras) - 03:09 4 nov 2024
- 49 was identified as a bow shock candidate, along with M17 in a study of Extended Red Objects (ERO's) and Stellar Wind Bow Shocks in the Carina nebula.…5 kB (498 palabras) - 11:20 22 sep 2024
- progenitor being a runaway star system. The bow shock is caused by the interaction of the advancing stellar wind with the interstellar medium. A remnant…16 kB (1679 palabras) - 19:20 17 oct 2024