• Thumbnail for Star formation
    Star formation is the process by which dense regions within molecular clouds in interstellar space, sometimes referred to as "stellar nurseries" or "star-forming...
    45 KB (5,279 words) - 18:55, 20 April 2024
  • Thumbnail for Neutron star
    through fusion, they inexorably cool down after their formation. Consequently, a given neutron star reaches a surface temperature of one million degrees...
    101 KB (11,799 words) - 02:44, 25 April 2024
  • clustered nature of star formation by treating star clusters as the fundamental unit of star formation. This approach permits the growth of star particles by...
    45 KB (5,608 words) - 07:05, 7 April 2024
  • Thumbnail for Star
    regions. Such feedback effects, from star formation, may ultimately disrupt the cloud and prevent further star formation. All stars spend the majority of...
    146 KB (16,321 words) - 21:30, 23 April 2024
  • Thumbnail for Binary star
    formation process. The observation of binaries consisting of stars not yet on the main sequence supports the theory that binaries develop during star...
    68 KB (8,144 words) - 11:36, 18 April 2024
  • Thumbnail for Nebular hypothesis
    not well known. Thus the formation of planetary systems is thought to be a natural result of star formation. A Sun-like star usually takes approximately...
    75 KB (9,132 words) - 21:19, 18 March 2024
  • Thumbnail for Molecular cloud
    (if star formation is occurring within), is a type of interstellar cloud, the density and size of which permit absorption nebulae, the formation of molecules...
    33 KB (3,729 words) - 09:11, 1 April 2024
  • Thumbnail for Elliptical galaxy
    clusters. Star formation activity in elliptical galaxies is typically minimal; they may, however, undergo brief periods of star formation when merging...
    17 KB (1,890 words) - 20:22, 16 April 2024
  • Thumbnail for Galaxy
    heavy elements, eventually allowing the formation of planets. Hubble eXtreme Deep Field (XDF) Star formation rates in galaxies depend upon their local...
    164 KB (16,377 words) - 17:18, 27 April 2024
  • Thumbnail for Cosmology
    cosmological constant. Absolute time and space Big History Earth science Galaxy formation and evolution Illustris project Jainism and non-creationism Lambda-CDM...
    51 KB (3,263 words) - 19:20, 24 April 2024
  • Thumbnail for Leo I (dwarf galaxy)
    major increase (accounting for 70% to 80% of its population) in its star formation rate between 6 Ga and 2 Ga (billion years ago). There is no significant...
    8 KB (891 words) - 22:23, 2 December 2023
  • Thumbnail for Starburst galaxy
    exceptionally high rate of star formation, as compared to the long-term average rate of star formation in the galaxy, or the star formation rate observed in most...
    19 KB (2,046 words) - 05:47, 11 March 2024
  • Thumbnail for Low-ionization nuclear emission-line region
    gas found in star formation regions. However, if star formation cannot be found in LINERs, then this definitively excludes star formation as powering LINER...
    11 KB (1,272 words) - 21:38, 12 August 2023
  • Thumbnail for Triangulum Galaxy
    "The Star Formation History of the Local Group". In F. Favata; A. Kaas; A. Wilson (eds.). Proceedings of the 33rd ESLAB symposium on star formation from...
    48 KB (5,110 words) - 05:08, 26 April 2024
  • Thumbnail for Timeline of the early universe
    parent star Kepler 452 7.98 billion years (5.82 Gya): Formation of Mira or Omicron ceti, binary star system. Formation of Alpha Centauri Star System,...
    36 KB (4,978 words) - 09:10, 17 April 2024
  • Thumbnail for Messier 100
    spots. Messier 100 is considered a starburst galaxy with the strongest star formation activity concentrated in its center, within a ring – actually two tightly...
    10 KB (1,085 words) - 09:17, 24 February 2024
  • Thumbnail for Whirlpool Galaxy
    period of enhanced star formation. The present efficiency of star formation, defined as the ratio of mass of new stars to the mass of star-forming gas, is...
    29 KB (2,982 words) - 23:59, 12 March 2024
  • Thumbnail for Star cluster
    leading to the disruption of a star cluster. Most young embedded clusters disperse shortly after the end of star formation. The open clusters found in the...
    21 KB (2,538 words) - 15:41, 22 April 2024
  • Thumbnail for Andromeda Galaxy
    sequence" (galaxies that lack star formation). Star formation activity in green valley galaxies is slowing as they run out of star-forming gas in the interstellar...
    108 KB (10,628 words) - 03:57, 22 April 2024
  • Thumbnail for Bok globule
    small dark nebulae containing dense cosmic dust and gas from which star formation may take place. Bok globules are found within H II regions, and typically...
    9 KB (842 words) - 09:43, 4 March 2024
  • Thumbnail for Milky Way
    Milky Way (section Formation)
    sequence" (galaxies that lack star formation). Star-formation activity in green valley galaxies is slowing as they run out of star-forming gas in the interstellar...
    209 KB (20,990 words) - 05:02, 21 April 2024
  • Thumbnail for Stellar population
    were later shown to be very important and were possibly related to star formation, observed kinematics, stellar age, and even galaxy evolution in both...
    35 KB (3,671 words) - 15:55, 29 April 2024
  • baryonic physics, gas heating and cooling, star formation and feedback. Understanding the processes of galaxy formation is a major topic of modern cosmology...
    27 KB (3,468 words) - 09:11, 2 June 2023
  • Thumbnail for Nebula
    Nebula (redirect from Nebulous star)
    Nebulae are often star-forming regions, such as in the "Pillars of Creation" in the Eagle Nebula. In these regions, the formations of gas, dust, and other...
    21 KB (2,844 words) - 07:15, 13 April 2024
  • Thumbnail for Spiral galaxy
    Spiral galaxy (redirect from Halo star)
    center into the galactic disc. The spiral arms are sites of ongoing star formation and are brighter than the surrounding disc because of the young, hot...
    30 KB (3,619 words) - 14:09, 19 April 2024
  • Thumbnail for O-type star
    O-like spectra. O-type stars are typically found in regions of active star formation, such as the spiral arms of a spiral galaxy or a pair of galaxies undergoing...
    30 KB (3,350 words) - 09:26, 22 April 2024
  • Thumbnail for Local Bubble
    for the formation of all young, nearby stars. These new stars are typically in molecular clouds like the Taurus molecular cloud and the open star cluster...
    20 KB (2,080 words) - 10:01, 26 January 2024
  • Thumbnail for Open cluster
    have been found only in spiral and irregular galaxies, in which active star formation is occurring. Young open clusters may be contained within the molecular...
    51 KB (6,248 words) - 01:28, 6 February 2024
  • Thumbnail for Messier 65
    of authors. The galaxy is low in dust and gas, and there is little star formation in it, although there has been some relatively recently in the arms...
    6 KB (491 words) - 06:59, 30 December 2023
  • Thumbnail for Quasi-star
    (25 May 2013). "Massive black hole factories: Supermassive and quasi-star formation in primordial halos". Astronomy & Astrophysics. 558: A59. arXiv:1305...
    9 KB (1,048 words) - 10:20, 18 April 2024