Close Menu
    Facebook X (Twitter) Instagram
    SciTechDaily
    • Biology
    • Chemistry
    • Earth
    • Health
    • Physics
    • Science
    • Space
    • Technology
    Facebook X (Twitter) Pinterest YouTube RSS
    SciTechDaily
    Home»Space»Astronomers Reveal Unified Model for Galactic Discs: Star Formation, Turbulence Driving, and Mass Transport
    Space

    Astronomers Reveal Unified Model for Galactic Discs: Star Formation, Turbulence Driving, and Mass Transport

    By Megan Watzke, Harvard-Smithsonian Center for AstrophysicsJuly 20, 20181 Comment3 Mins Read
    Facebook Twitter Pinterest Telegram LinkedIn WhatsApp Email Reddit
    Share
    Facebook Twitter LinkedIn Pinterest Telegram Email Reddit
    A Unified Model for Galactic Discs
    A Hubble image of the spiral disc galaxy NGC3972. Astronomers have developed a new model to explain why the star formation rate in nearly all disk galaxies, including the Milky Way, is so small, and why it correlates in the same way with a galaxy’s gas mass and motions. NASA/Hubble

    Disc galaxies like our own Milky Way, characterized by a flattened disc of stars and gas (often with a central bulge of material as well) have a wide range of masses, spatial extents, and stellar content. Nonetheless all disc galaxies, both locally and in the distant Universe, share some strikingly similar properties. Most notable is that the star formation rate correlates tightly with the galaxy’s gas content, the gas motions (the “velocity dispersion”), and the dynamical lifetime (roughly, the time it takes for the galaxy to rotate once). Moreover, this curiously universal rate is remarkably small: only about one percent of the gas in disc galaxies turns into stars over that timescale, with much of the activity concentrated in the galaxies’ central regions. Most simple models of star formation predict that gravity should be much more effective in forming stars as it compresses the gas in molecular clouds. Observations indicate that both the correlations and the inefficiency extend down to the scale of individual molecular clouds.

    CfA astronomers Blakesley Burkhart and John Forbes and two colleagues have developed a new unified model for galaxy discs that explains these phenomena, and some others besides. The scientists show that the correlation of star formation rate with gas motion is not caused by these motions but rather is the result of the transport of material within the galaxy, which affects both. The model maintains a state of gas equilibrium and marginal gravitational stability by including in a galaxy the radial transport of gas towards its nucleus and also the turbulent feedback from star formation. These two considerations are relatively straightforward in principle but produce a dramatic improvement in the agreement between observations and theory, for example by explaining how the eventual quenching of the star formation happens. The new work also provides a natural explanation for the cosmic epochs at which galaxies build up bulges and discs.

    Reference(s): “A Unified Model for Galactic Discs: Star Formation, Turbulence Driving, and Mass Transport” by Mark R. Krumholz, Blakesley Burkhart, John C. Forbes and Roland M. Crocker, 5 April 2018,  MNRAS.
    DOI: 10.1093/mnras/sty852

    Never miss a breakthrough: Join the SciTechDaily newsletter.
    Follow us on Google and Google News.

    Astronomy Astrophysics Harvard-Smithsonian Center for Astrophysics
    Share. Facebook Twitter Pinterest LinkedIn Email Reddit

    Related Articles

    X-Ray Emission From Mysterious Dark Matter

    Analyzing Dust Storm Sequences on Mars

    Intriguing Remains of a Rare Stellar Explosion Discovered in Milky Way Center

    Puzzling Astrophysics of Quasars in the Early Universe

    Four Exoplanets – Including a Super-Earth Planet – Discovered by High School Students

    Massive Rotating Stars in the Pleiades Cluster

    Astronomers Discover First Cloudless, Jupiter-Like Planet – “Smoking Gun Evidence”

    Chandra X-ray Observatory Studies Extraordinary Magnetar [Video]

    Chandra Studies Extraordinary Magnetar: Fastest Spinning and Possibly the Youngest Magnetar Known

    1 Comment

    1. Kopernik on August 29, 2019 1:44 pm

      “Astronomers Reveal Unified Model for Galactic Discs: Star Formation, Turbulence Driving, and Mass Transport”

      Reply
    Leave A Reply Cancel Reply

    • Facebook
    • Twitter
    • Pinterest
    • YouTube

    Don't Miss a Discovery

    Subscribe for the Latest in Science & Tech!

    Trending News

    FDA-Approved Drug Shows Promise for Reversing Osteoarthritis Damage

    11,000-Year-Old Grains Reveal a Surprise About the Origins of Agriculture

    This Common Type of Medication Is Linked to Slower Cognitive Decline

    Quantum Computer Solves a Problem in 15 Minutes That Classical Methods Can’t Practically Compute

    Taking the Stairs Could Cut Your Risk of Heart-Related Death by 39%

    Scientists Uncover a Surprising New Route for Stonehenge’s Most Mysterious Stone

    A Star Near the Milky Way’s Black Hole Is Losing Mass at an Astonishing Rate

    Scientists Solve a Vitamin B12 Mystery With an Unexpected Culprit

    Follow SciTechDaily
    • Facebook
    • Twitter
    • YouTube
    • Pinterest
    • Newsletter
    • RSS
    SciTech News
    • Biology News
    • Chemistry News
    • Earth News
    • Health News
    • Physics News
    • Science News
    • Space News
    • Technology News
    Recent Posts
    • Natural Compound in Broccoli Could Help Treat a Rare, Incurable Neurological Disease
    • Common Supplements Show Antibiotic-Like Benefits Against Severe Gum Disease
    • Scientists Warn of a Nearly 400% Increase in Toxic Liver Injuries – One Common Drug Leads the List
    • Earth-Like Worlds Could Have Formed Billions of Years Earlier Than Scientists Thought
    • “I Jumped From My Chair” – Astronomers Discover a Hidden Star Orbiting Betelgeuse
    Copyright © 1998 - 2026 SciTechDaily. All Rights Reserved.
    • Science News
    • About
    • Contact
    • Editorial Board
    • Privacy Policy
    • Terms of Use

    Type above and press Enter to search. Press Esc to cancel.