star formation tagged posts

Star Formation in Distant Galaxy Clusters

Star formation in distant galaxy clusters

The galaxy cluster Abell 1689 as seen by Hubble. The mass in the cluster acts as a gravitational lens, distorting the light from background galaxies into blueish arcs of light. Abell 1689 is relatively close by, but astronomers have now spotted clusters in the early universe via their lensing of even more remote, luminous galaxies, and have studied the star formation underway in their outer regions. Credit: NASA, N. Benitez (JHU), T. Broadhurst (Racah Institute of Physics/The Hebrew University), H. Ford (JHU), M. Clampin (STScI), G. Hartig (STScI), G. Illingworth (UCO/Lick Observatory), the ACS Science Team and ESA

The first stars appeared ~100 million years after the big bang, and ever since then stars and star formation processes have lit up the cosmos, producing heavy elements, planets,...

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Star Formation in the Outskirts of Galaxies

Star formation in the outskirts of galaxies

Star formation in the outer spiral regions of the galaxy NGC 4625 is seen in ultraviolet light (blue); these arms are nearly invisible in optical light, but have hot, newborn stars that radiate in the UV. A new study finds that the star formation processes in these outer regions generally resemble the processes at work in more normal, denser regions where molecular gas abounds. The atomic gas is traced in the radio (purple); optical starlight is red. Credit: NASA/JPL-Caltech/Carnegie Observatories/WSRT

Star formation environments can be roughly grouped into 3 types, categorized by the density of their gas (or more precisely, the projected “surface” density of the gas, which is easier to determine than volume density)...

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3D Visualisation Redefines Milky Way’s local Architecture

Another Dimension: 3D visualisation redefines Milky Way's local architecture

Visualising the local solar neighbourhood in 3D. Credit: ESA. Acknowledgement: H. Bouy (CSIC-INTA) & J. Alves (U. Vienna

Astronomers have used modern techniques to visualise data from ESA’s Hipparcos space astrometry mission in 3D. This offered insights into the distribution of nearby stars and uncovered new groupings of stars in the solar neighbourhood, shedding light on the origins of the stars in Orion and calling into question the existence of the Gould Belt – an iconic ring-shaped structure of stars in the Milky Way. The results show the potential of 3D visualisation of the solar neighbourhood, an approach which is of particular relevance to ESA’s Gaia mission which will map the Milky Way and Local Group in 3D with unprecedented sensitivity and accuracy.

3D map of massive O and B ty...

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Peering into Building Blocks of Galaxies

Peering into building blocks of galaxies

An image of Camargo 791, one of the newly found embedded clusters. Credit: Camargo et al.

When a giant cloud of molecular gas condenses, star clusters are born. It may sound simple but the formation of star clusters is a very complex process. By peering into this process we could get valuable information on the evolution of galaxies and improve our knowledge about large cosmic structures in the universe. “Star clusters are often considered as building blocks of galaxies. Understanding how these objects form and evolve is vital to our comprehension of the structure, formation and evolution of galaxies,” Denilso Camargo.

Camargo and his colleagues recently discovered a multitude of star clusters using NASA’s Wide-field Infrared Survey Explorer: 652 star clusters, stellar groups and candidate...

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