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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 (2474 palabras) - 11:52 4 jun 2024
Resultados de la Wikipedia en inglés.
- bow-shocks in the galactic plane. This larger catalog will help to understand the stellar wind of massive stars. The closest stars with infrared bow-shocks…18 kB (2030 palabras) - 17:42 13 ene 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 (2381 palabras) - 01:58 18 may 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…61 kB (6406 palabras) - 15:25 20 may 2024
- ; Stevens, I. R.; Isequilla, N. L. (2012). "E-BOSS: An Extensive stellar BOw Shock Survey. I. Methods and first catalogue". Astronomy & Astrophysics…39 kB (4689 palabras) - 01:46 5 may 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
- 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 (4800 palabras) - 23:13 6 jun 2024
- 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…172 kB (18 256 palabras) - 15:06 6 jun 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
- 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 (1874 palabras) - 11:09 7 mar 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) - 20:38 3 feb 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) - 13:51 24 abr 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 (1666 palabras) - 13:58 6 sep 2023
- 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…37 kB (4063 palabras) - 11:44 9 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 (7047 palabras) - 17:33 13 abr 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 (1675 palabras) - 13:02 20 may 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 (878 palabras) - 08:16 15 ago 2023
- 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) - 04:19 14 may 2024
- Radiation zone (sección Eddington stellar model)An Introduction to Stellar Astrophysics (1st ed.), John Wiley and Sons, p. 168, ISBN 978-1-119-96497-1 O.R. Pols (2011), Stellar Structure and Evolution…11 kB (1718 palabras) - 19:15 4 abr 2024
- Kelvin–Helmholtz instability. The solar wind is supersonic and passes through a bow shock where the direction of flow is changed so that most of the solar wind…13 kB (1625 palabras) - 21:50 13 dic 2023