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Formation of Species

Speciation describes the formation of one or more new species from one or sometimes multiple original species. The resulting species are discrete from the parent species, and barriers to reproduction will typically exist. There are two primary mechanisms, speciation with and without geographic isolation—allopatric and sympatric speciation, respectively.
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Related Experiment Video

Updated: May 12, 2026

Bringing the Visible Universe into Focus with Robo-AO
10:35

Bringing the Visible Universe into Focus with Robo-AO

Published on: February 12, 2013

Massive star formation within the Leo 'primordial' ring.

David A Thilker1, Jennifer Donovan, David Schiminovich

  • 1Center for Astrophysical Sciences, The Johns Hopkins University, 3400 North Charles Street, Baltimore, Maryland 21218, USA. dthilker@pha.jhu.edu

Nature
|February 20, 2009
PubMed
Summary
This summary is machine-generated.

The Leo ring, a massive gas cloud, shows signs of recent star formation, suggesting it may be a forming dwarf galaxy. This discovery offers insights into early universe galaxy formation. Keywords: Leo ring, star formation, dwarf galaxies, galaxy formation.

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Related Experiment Videos

Last Updated: May 12, 2026

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Published on: February 12, 2013

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Published on: November 6, 2018

Area of Science:

  • Astronomy and Astrophysics
  • Cosmology
  • Galaxy Formation and Evolution

Background:

  • Intergalactic neutral atomic hydrogen (H i) clouds are rare in the local Universe, with few primordial examples found.
  • The Leo ring, a massive H i structure, is a candidate for such a primordial cloud, previously only observed via H i emission.

Purpose of the Study:

  • To investigate the Leo ring for evidence of a stellar population and ongoing star formation.
  • To characterize the properties of any detected stellar populations, including metallicity and formation timescale.

Main Methods:

  • Detection of ultraviolet light from gaseous substructures within the Leo ring.
  • Analysis of ultraviolet-visible photometry to constrain metallicity and star formation duration.

Main Results:

  • Detection of ultraviolet light, indicating recent massive star formation within the Leo ring's gaseous substructures.
  • The observed ultraviolet color suggests a star formation burst or moderate continuous star formation (approx. 10^8 years).
  • Photometry favors low metallicity models (Z approx. Z☉/50-Z☉/5), requiring spectroscopic confirmation.

Conclusions:

  • The Leo ring's substructures may represent forming dwarf galaxies lacking dark matter, akin to tidal dwarf galaxies but without prior enrichment.
  • If common in the early Universe, such structures could account for a significant population of undetected faint, metal-poor, halo-lacking dwarf galaxies.