Small Magellanic Cloud tagged posts

Nube, the Almost Invisible Galaxy that Challenges the Dark Matter Model

Nube, the almost invisible galaxy that challenges the dark matter model
The Nube galaxy. The figure is a composition of a color image and a black and white image, to pick out the background. Credit: GTC/Mireia Montes

Nube is an almost invisible dwarf galaxy discovered by an international research team led by the Instituto de Astrofísica de Canarias (IAC) in collaboration with the University of La Laguna (ULL) and other institutions.

The name was suggested by the 5-year-old daughter of one of the researchers in the group and is due to the diffuse appearance of the object. Its surface brightness is so faint that it had passed unnoticed in the various previous surveys of this part of the sky due to the object’s diffuse appearance as if it were some kind of ghost...

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New study shows Small Magellanic Cloud is actually Two Smaller Galaxies

Top: Intensity-weighted mean velocity map of the SMC from Pingel et al (2022). The single contour indicates an Hi column density of 15×1020⁢cm−2. The center of the SMC used in this work (defined based on the stellar populations observed by Gaia Zivick et al, 2021) is marked with a magenta cross. Spatial bins are overlaid and identified with numbers. Bottom: The average Hi brightness temperature spectra (Tb⁢(vr)) profiles from spatial bins marked at left (black). Each panel includes shaded gray envelopes denoting the 16th through 84th percentile of the Tb⁢(vr) within each spatial bin. We observe that the radial velocity structure of Hi emission features multiple, distinct velocity peaks (and typically two, dominant components). Credit: arXiv (2023). DOI: 10.48550/arxiv.2312...
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Study of Small Magellanic Cloud suggests Planets could have Formed during ‘Cosmic Noon’

Study of Small Magellanic Cloud suggests planets could have formed during 'cosmic noon'
NIRCam mosaics of NGC 346. Credit: Nature Astronomy (2023). DOI: 10.1038/s41550-023-01945-7

An international team of space scientists has found evidence suggesting that planets could have formed during the so-called “cosmic noon.” In their study, reported in the journal Nature Astronomy, the group used data from the James Webb Space Telescope (JWST) to study a part of the Small Magellanic Cloud (SMC) to learn more about planet development around young stars.

For many years, astronomers have been studying planet creation and the likelihood of the existence of planets similar to Earth. But it is still not clear how planets could have could come to exist in the early universe when most, if not all of the stars, were small...

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ALMA discovers Birth Cry from a Baby Star in the Small Magellanic Cloud

Researchers at Osaka Metropolitan University have observed “baby stars” in the Small Magellanic Cloud, having an environment similar to the early universe. Toward one of the baby stars, they found molecular outflow, which has similar properties to those seen in the Milky Way galaxy, giving a new perspective on the birth of stars.

The heavy elements in interstellar matter significantly impact the mechanism of star formation. In the early universe, the abundance of heavy elements was lower than in the present universe because there was not enough time for nucleosynthesis to produce heavy elements in stars. It has not been well understood how star formation in such an environment differs from present-day star formation.

An international team led by Professor Toshikazu Onishi, Osaka...

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