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Crab Nebula.» Astrophysical Journal Letters, vol. 373, pp. L59-L62. 1 de junio de 1991. Virginia Trimble, «Motions and Structure of the Filamentary Envelope…28 kB (3550 palabras) - 09:51 27 dic 2023
Resultados de la Wikipedia en inglés.
- remnant. More recent observations in the [SII] band also revealed fine filamentary structures within the shell that had not previously been seen. A 2021…12 kB (1474 palabras) - 01:09 11 may 2024
- regions using a coronagraph. The nebulosities were found to have "linear, filamentary, striated morphological structure" located between 1000 and 100,000 astronomical…2 kB (235 palabras) - 10:18 2 feb 2024
- and x-rays. In modern usage, the names Veil Nebula, Cirrus Nebula, and Filamentary Nebula generally refer to all the visible structure of the remnant, or…13 kB (1319 palabras) - 14:03 17 abr 2024
- Molecular cloud (categoría Nebulae)of interstellar cloud, the density and size of which permit absorption nebulae, the formation of molecules (most commonly molecular hydrogen, H2), and…33 kB (3729 palabras) - 19:16 22 may 2024
- stripped hydrogen gas away from all three galaxies, forming gaseous filamentary structures in the group. Moreover, these interactions have allowed interstellar…23 kB (2045 palabras) - 18:49 31 may 2024
- H II region (categoría Nebulae)associated with giant molecular clouds. They often appear clumpy and filamentary, sometimes showing intricate shapes such as the Horsehead Nebula. H II…35 kB (4404 palabras) - 20:25 31 mar 2024
- Supercluster under Laniakea. Beginning with the first large sample of nebulae published by William and John Herschel in 1863, it was known that there…17 kB (1546 palabras) - 21:22 22 may 2024
- NGC 5189 (categoría Planetary nebulae)SABIN L.; VAZQUEZ R.; LOPEZ J.A.; GARCIA-DIAZ M.T.; et al. (2012). "The filamentary multi-polar planetary nebula NGC 5189" (PDF). Rev. Mex. Astron. Astrofís…5 kB (496 palabras) - 14:24 30 sep 2023
- Mz 3 (categoría Planetary nebulae)nebulosities are described as: two spherical bipolar lobes, two outer large filamentary hour-glass shaped columns, two cone shaped rays, and a planar radially…10 kB (1069 palabras) - 16:20 9 may 2024
- proposed such as a single spiral arm or a flocculent pattern of long, filamentary, and thick spiral arms. The most likely cause of the distortions of the…108 kB (10 640 palabras) - 16:03 3 jun 2024
- William Herschel on April 3, 1785. In 1943, this galaxy was one of six nebulae listed by American astronomer Carl Keenan Seyfert that showed broad emission…10 kB (1033 palabras) - 00:20 3 dic 2023
- NGC 6445 (categoría Planetary nebulae)~ 80°, stretching to about 1'.6 from the center. There are also many filamentary structures across the nebula, which hint at a more complex morphology…11 kB (1297 palabras) - 13:08 5 mar 2024
- Tanaka, T.; et al. (2011). "The Dynamical State of the Serpens South Filamentary Infrared Dark Cloud". Astrophysical Journal. 778 (1): 34. arXiv:1309…15 kB (1551 palabras) - 14:20 1 mar 2024
- hinders the galaxy from forming diffuse nebulae except through mergers with other galaxies. In the dense nebulae where stars are produced, much of the hydrogen…45 kB (5263 palabras) - 18:55 20 abr 2024
- Despite this, recent high-resolution images of its dusty disk show unusual filamentary patterns. These patterns are extending into the halo of the galaxy, away…11 kB (1041 palabras) - 16:19 3 may 2024
- Additionally, spiral arms are subdivided into two categories: massive and filamentary. In the first instance, the spiral arms are wide, diffuse, and do not…51 kB (5539 palabras) - 22:35 31 may 2024
- disc-shaped galaxy of stars. By the 20th century, observations of spiral nebulae revealed that the Milky Way galaxy was one of billions in an expanding…34 kB (1979 palabras) - 09:13 18 abr 2024
- NGC 6334 (categoría Emission nebulae)approximately 5.5 kilolight-years from the Sun. The nebula is a high mass filamentary cloud structure spanning ~320 ly. In the visible part of the spectrum…8 kB (568 palabras) - 16:10 3 feb 2024
- complex, or Taurus dark clouds, a star-forming region containing sparse, filamentary clouds of gas and dust. This spans a diameter of 98 light-years (30 parsecs)…38 kB (3896 palabras) - 19:11 9 may 2024
- stars are formed from collapsing clouds of gas and dust, often called nebulae or molecular clouds. Over the course of millions of years, these protostars…49 kB (6408 palabras) - 15:52 29 may 2024
- Bibcode:1990BAAS...22..832D. Grydeland, T. (2003). "Interferometric observations of filamentary structures associated with plasma instability in the auroral ionosphere"…62 kB (6403 palabras) - 20:19 12 may 2024