Galaxies

Blogs about galaxies, singles ones on in clusters

The galaxy JADES-GS-z13-1 (the red circle in the center) as seen by the James Webb Space Telescope (Image ESA/Webb, NASA, STScI, CSA, JADES Collaboration, Brant Robertson (UC Santa Cruz), Ben Johnson (CfA), Sandro Tacchella (Cambridge), Phill Cargile (CfA), J. Witstok, P. Jakobsen, A. Pagan (STScI), M. Zamani (ESA/Webb))

0

An article published in the journal “Nature” reports the results of observations of the primordial galaxy cataloged as JADES-GS-z13-1. A team of researchers used the James Webb Space Telescope to examine this galaxy, estimating that it dates back to about 330 million years after the Big Bang. The surprise came from spectroscopic analyses with so-called Lyman-alpha radiation, emitted in the ultraviolet by hydrogen in specific circumstances, because it was much stronger than would be expected from a galaxy of that era.

Herbig-Haro 49/50 (NIRCam and MIRI Image, annotated)

0

An image captured by the James Webb Space Telescope shows Herbig-Haro 49/50, or simply HH 49/50, a type of nebula associated with star formation. The Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI) instruments were used in combination to observe infrared details of the outflows whose shape led to the object being nicknamed the Cosmic Tornado. For years, astronomers have wondered what the object they could barely see in images obtained with other instruments at the “tip of the tornado” was, and Webb helped them realize that it’s a spiral galaxy that is far more distant.

The Small Magellanic Cloud and the molecular coulds subject of this study

0

An article published in “The Astrophysical Journal” reports a study of 17 molecular clouds in the Small Magellanic Cloud, one of the Milky Way’s satellite dwarf galaxies. A team of researchers led by Kazuki Tokuda, a postdoctoral researcher at Kyushu University, Japan, examined high-resolution images captured using the ALMA radio telescope to obtain information on their characteristics. The examination showed that 40% of those clouds had a more diffused gas, with fluffy structures. The others were classic molecular clouds with a filamentary structure that are also found in the Milky Way. This difference was attributed to the scarcity of elements heavier than hydrogen and helium in the Small Magellanic Cloud, a situation similar to that of the early universe.

Mosaic of candidate active galactic nuclei in dwarf galaxie

0

An article to be published in “The Astrophysical Journal” reports the discovery of about 2,500 new candidate active galactic nuclei in dwarf galaxies and about 300 new candidate intermediate-mass black holes. A team of researchers examined observations conducted with the Dark Energy Spectroscopic Instrument (DESI) on the Nicholas U. Mayall 4-meter Telescope in Arizona to find all these possible black holes.

The Einstein ring around galaxy NGC 6505 (Image ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre, G. Anselmi, T. Li / CC BY-SA 3.0 IGO)

0

An article published in the journal “Astronomy & Astrophysics” reports the identification of a practically perfect so-called Einstein ring around the galaxy NGC 6505. A team of researchers Conor led by O’Riordan of the Max Planck Institute for Astrophysics in Munich, Germany, examined observations conducted with the Euclid space telescope to study the image of a much more distant galaxy distorted by the gravitational lens created by NGC 6505. This effect allows to study NGC 6505 as well because its mass creates that gravitational lens, so its effects allow to analyze it.