Analysis
of early galaxies in the Hubble deep fields taken near the north and south celestial poles (in 1995 and 1998, respectively) suggest that the farthest objects in the deep fields are only the «tip of the iceberg» of a uniquely effervescent period of star birth.
Astronomers now have very strong evidence that the peculiar
colors of early galaxies seen in the Spitzer Space Telescope images originate from a very rapid formation of massive, young stars, which interacted with the primordial gas in these galaxies.
Astronomers now have very strong evidence that the peculiar colors
of early galaxies seen in the Spitzer images originate from a very rapid formation of massive, young stars, which interacted with the primordial gas in these galaxies.
Another major finding of this study was the systematic detection of luminous hydrogen halos around galaxies in the early Universe, giving astronomers a new and promising way to study how material flows in and
out of early galaxies.
If confirmed, the finding means that some of the universe's first stars were so massive they died in exceptionally violent explosions that altered the
growth of early galaxies.
The study is «an important step forward» in understanding the
evolution of early galaxies, says astronomer Giovanni Fazio of the Harvard - Smithsonian Center for Astrophysics in Cambridge, Massachusetts.
«Vast luminous nebula poses a cosmic mystery: Glowing nebula found at the heart of a huge «rotocluster»
of early galaxies appears to be part of the cosmic web of filaments connecting galaxies, but what's lighting it up?.»
Researchers found this massive
overdensity of early galaxies, called a «protocluster,» through a novel survey project led by Zheng Cai, a Hubble Postdoctoral Fellow at UC Santa Cruz.
Astronomers now have strong evidence that the peculiar
colors of early galaxies — seen in the Spitzer images — originate from a rapid formation of massive, young stars, which interacted with the primordial gas in these galaxies.
«MUSE has the unique ability to extract information about
some of the earliest galaxies in the Universe — even in a part of the sky that is already very well studied,» explains Jarle Brinchmann, lead author of one of the papers describing results from this survey, from the University of Leiden in the Netherlands and the Institute of Astrophysics and Space Sciences at CAUP in Porto, Portugal.
Astronomer Matt Mountain, director of the new Gemini Telescope in Hawaii, says this future generation of gargantuan earthbound telescopes would make it possible to study individual stars in
some of the earliest galaxies or determine the atmospheric gases of distant planets.
Astronomers have looked back to a time soon after the Big Bang, and have discovered swirling gas in
some of the earliest galaxies to have formed in the Universe.
These events occur disproportionately often in dwarf irregular galaxies, which are thought to be similar to
some of the earliest galaxies that populated the universe.