• Thumbnail for Hydrogen-alpha
    Hydrogen-alpha (redirect from )
    Hydrogen-alpha, typically shortened to H-alpha or , is a deep-red visible spectral line of the hydrogen atom with a wavelength of 656.28 nm in air and...
    7 KB (856 words) - 14:17, 7 April 2024
  • {\displaystyle \ldots } Or, directly again from the derived definition, () = α(()). If α expresses a "computational step" computed by αρν for some ρ...
    17 KB (2,338 words) - 22:45, 19 March 2024
  • Thumbnail for Solar flare
    the observation of not very bright flares with small telescopes. For years was the main, if not the only, source of information about solar flares. Other...
    43 KB (4,451 words) - 07:05, 18 May 2024
  • Thumbnail for Karl Gordon Henize
    Scientific Achievement Medal in 1974. In 1956, Henize published the Catalogues of -Emission Stars and Nebulae in the Magellanic Clouds. The paper references...
    17 KB (1,889 words) - 04:02, 21 March 2024
  • Thumbnail for California Nebula
    extremely difficult to observe visually. It can be observed with a filter (isolates the line at 656 nm) or Hβ filter (isolates the Hβ line at 486 nm)...
    3 KB (251 words) - 01:33, 26 January 2024
  • Thumbnail for ChaHα8
    ChaHα8 (redirect from Cha 8)
    "Improved radial velocity orbit of the young binary brown dwarf candidate Cha 8". Astronomy and Astrophysics. 521 (A24): A24. arXiv:1006.2383. Bibcode:2010A&A...
    4 KB (284 words) - 02:23, 7 May 2024
  • Thumbnail for Moreton wave
    ejections accelerate shocks. Moreton waves can be observed primarily in the band. Asteroseismology Gravity wave Helioseismology OSO 8 Solar prominence...
    6 KB (562 words) - 19:02, 13 August 2023
  • Thumbnail for T Coronae Borealis
    1086/301260. Stanishev, V.; Zamanov, R.; Tomov, N.; Marziani, P. (2004). " variability of the recurrent nova T Coronae Borealis". Astronomy and Astrophysics...
    14 KB (1,345 words) - 13:59, 9 May 2024
  • Thumbnail for Rigel
    measured to vary by about 10 km/s around a mean of 21.5 km/s. In 1933, the line in Rigel's spectrum was seen to be unusually weak and shifted 0.1 nm...
    72 KB (7,280 words) - 19:11, 3 May 2024
  • Thumbnail for Interstellar medium
    L.; Madsen, G. J.; Jaehnig, K. P.; Percival, J. W. (2003), "The Wisconsin Mapper Northern Sky Survey", Astrophysical Journal Supplement, 145 (2): 405...
    60 KB (7,342 words) - 02:22, 17 May 2024
  • ultraviolet, white light, and are sometimes referred to as X-ray jets, EUV jets, white-light jets, and jets (or surges), respectively. Since ejected...
    5 KB (540 words) - 13:46, 17 May 2024
  • Thumbnail for Brown dwarf
    "16–20 MJup Radial Velocity Companion Orbiting the Brown Dwarf Candidate Cha 8". The Astrophysical Journal. 666 (2): L113–L116. arXiv:0707.3744. Bibcode:2007ApJ...
    185 KB (20,085 words) - 16:16, 16 May 2024
  • Thumbnail for Seyfert galaxy
    component in the line, and not in higher order Balmer lines. In Type 1.8, very weak broad lines can be detected in the Hβ lines as well as , even if they...
    49 KB (5,702 words) - 16:00, 6 May 2024
  • Thumbnail for NGC 1579
    NGC 1579 (redirect from Lk 101)
    region of star formation. The star cluster contains the emission-line star Lk 101, which provides much of the ionizing radiation in the nebula. NGC 1579...
    3 KB (261 words) - 03:32, 15 August 2023
  • Thumbnail for Ellerman bomb
    brightenings in the Sun's photosphere. They are only observed in the wings of the , Hβ, and Hγ hydrogen spectral lines and take place in emerging flux regions...
    4 KB (469 words) - 19:12, 4 April 2024
  • Thumbnail for Horsehead Nebula
    Colour images reveal a red colour that originates from ionised hydrogen gas () predominantly behind the nebula, and caused by the nearby bright star Sigma...
    9 KB (852 words) - 22:59, 19 May 2024
  • Thumbnail for Coronal hole
    ISBN 0-521-59264-X. Jiang, Y., Chen, H., Shen, Y., Yang, L., & Li, K. (2007, January). dimming associated with the eruption of a coronal sigmoid in the quiet Sun...
    6 KB (613 words) - 20:14, 12 May 2024
  • Thumbnail for Chromosphere
    chromosphere has a characteristic red color due to electromagnetic emissions in the spectral line. Information about the chromosphere is primarily obtained by...
    12 KB (1,304 words) - 15:09, 11 April 2024
  • Thumbnail for List of most massive black holes
    from quasar line correlation. Another paper suggests much higher masses of (8.318±0.6)×1010 M☉ and 8.511+2.2 −1.8×1010 M☉ based on and Hβ line correlations...
    76 KB (5,741 words) - 23:14, 1 May 2024
  • Thumbnail for Henize 70
    supernova remnants due to having similar SII/ line ratios although most supernova remnants have higher NII/ line ratios. Using angular dimensions of 7’...
    12 KB (1,176 words) - 17:41, 2 May 2024
  • Thumbnail for Taylor's theorem
    continuously differentiable function at the point a ∈ Rn. Then there exist functions  : Rn → R, where | α | = k , {\displaystyle |\alpha |=k,} such that f ( x )...
    54 KB (9,621 words) - 12:42, 27 March 2024
  • coordinate system Ha, or alternative hypothesis, in statistical testing H-alpha (), a deep-red visible spectral line of the hydrogen atom Ha (Chinese surname)...
    4 KB (428 words) - 10:47, 27 April 2024
  • Thumbnail for Cassiopeia (constellation)
    & Tirion 2001, pp. 106–108. Catanzaro, G. (2013). "Spectroscopic atlas of and Hβ in a sample of northern Be stars". Astronomy & Astrophysics. 550 (A79):...
    39 KB (4,689 words) - 01:46, 5 May 2024
  • Thumbnail for Orion Nebula
    addition to regions of red and of blue-violet. The red hue is a result of the recombination line radiation at a wavelength of 656.3 nm. The blue-violet...
    45 KB (4,799 words) - 05:54, 19 April 2024
  • Thumbnail for Stellar corona
    the Sun's surface: sunspots and faculae occur in the photosphere; spicules, filaments and plages in the chromosphere; prominences in the chromosphere...
    62 KB (7,681 words) - 04:04, 2 May 2024
  • is the unilateral shift on a Hilbert space , and U is a unitary operator (possible vacuous). The family {} consists of isomorphic Hilbert spaces. A...
    8 KB (1,123 words) - 04:10, 1 May 2024
  • Thumbnail for Proxima Centauri
    Hugh R. A.; Barnes, John R. (June 2017). "Calculations of periodicity from profiles of Proxima Centauri". Astronomy & Astrophysics. 602. A48. arXiv:1608...
    102 KB (10,204 words) - 11:28, 9 May 2024
  • Thumbnail for Fourier-transform infrared spectroscopy
    0.1 cm−1 resolution. Michelson himself attempted to resolve the hydrogen emission band in the spectrum of a hydrogen atom into its two components by...
    37 KB (4,750 words) - 10:26, 27 April 2024
  • Thumbnail for Messier 81
    J.; Su, K. Y. L.; Young, E. T. (2004). "Spatially Resolved Ultraviolet, , Infrared, and Radio Star Formation in M81". Astrophysical Journal Supplement...
    23 KB (2,045 words) - 22:40, 1 March 2024
  • Wright, N.; Zijlstra, A. A.; Zurita, A. (September 2005). "The INT Photometric Survey of the Northern Galactic Plane (IPHAS)". Monthly Notices of the Royal...
    5 KB (507 words) - 10:29, 5 January 2024