Astronomers detect first stars “bubbling out” from the cosmic dark ages
oir2001a – Rendition of the galaxy group EGS77
This rendition shows ionized bubbles formed by three galaxies in galaxy cluster EGS77.
Credit: V. Tilvi et al./National Science Foundation’s Optical-Infrared Astronomy Research Laboratory/KPNO/AURA
Astronomers using the Mayall telescope at Kitt Peak National Observatory, a program of NSF’s National Optical-Infrared Astronomy Research Laboratory, have identified several overlapping bubbles of hydrogen gas ionized by the stars in early galaxies, a mere 680 million years after the Big Bang. This is the earliest direct evidence from the period when the first generation of stars formed and began reionizing the hydrogen gas that permeated the Universe.
There was a period in the very early Universe — known as the “cosmic dark ages” — when elementary particles, formed in the Big Bang, had combined to form neutral hydrogen but no stars or galaxies existed yet to light up the Universe. This period began less than half a million years after the Big Bang and ended with the formation of the first stars. While this stage in the evolution of our Universe is indicated by computer simulations, direct evidence is sparse.
Now, astronomers using the infrared imager NEWFIRM on the 4-meter Mayall Telescope at the Kitt Peak National Observatory of NSF’s National Optical-Infrared Astronomy Research Laboratory (NOIRLab), have reported imaging a group of galaxies, known as EGS77 , that contains these first stars. Their results were announced at a press conference held today at the 235th meeting of the American Astronomical Society (AAS) in Honolulu, Hawai‘i.
“The young Universe was filled with hydrogen atoms, which so attenuate ultraviolet light that they block our view of early galaxies,” said James Rhoads at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, who presented the findings at the AAS press conference. “EGS77 is the first galaxy group caught in the act of clearing out this cosmic fog.”
The team began with an imaging survey designed to detect high redshift galaxies and combined these data with corresponding images taken by the Hubble Space Telescope. This enabled the team to compute what is known as a photometric redshift, a proxy for estimating distance. At these redshifts, a galaxy’s light is shifted completely out of the range of wavelengths to which the human eye is sensitive (the visible spectrum) to longer (infrared) wavelengths. The criteria for selecting distant galaxy candidates included a clear detection of them in the special infrared narrowband filters used with NEWFIRM on the Mayall 4-meter telescope and a complete non-detection in the shorter wavelength optical filter bands used by Hubble. “The discovery of the two fainter galaxies in the group was only possible because of the special narrowband filter used with NEWFIRM,” said team leader Vithal Tilvi, a researcher at Arizona State University in Tempe.
“Intense light from galaxies can ionize the surrounding hydrogen gas, forming bubbles that allow starlight to travel freely,” said Tilvi. “EGS77 has formed a large bubble that allows its light to travel to Earth without much attenuation. Eventually, bubbles like these grew around all galaxies and filled intergalactic space, clearing the way for light to travel across the Universe.”
EGS77 was discovered as part of the Cosmic Deep And Wide Narrowband (Cosmic DAWN) survey, for which Rhoads serves as principal investigator. The team imaged a small area in the constellation of Boötes using a custom-built filter on the National Optical Astronomy Observatory’s Extremely Wide-Field InfraRed imager (NEWFIRM). Ron Probst, a DAWN team member who also helped to develop NEWFIRM, adds, “These results show the value of maintaining instruments at our national observatories that are powerful and can flexibly adapt to pursue new scientific questions, questions that may not have been in mind when an instrument was originally built.”
Once identified, the distances and hence the ages of these galaxies were confirmed with spectra taken with the MOSFIRE spectrograph at the Keck I telescope at the W. M. Keck Observatory on Maunakea in Hawai‘i. All three galaxies show strong emission lines of hydrogen Lyman alpha at a redshift (z = 7.7), which means we are seeing them at about 680 million years after the Big Bang. The size of the ionized bubble around each was derived from computer modeling. These bubbles overlap spatially, but are large enough (about 2.2 million light-years) that Lyman alpha photons are redshifted before they reach the boundary of the bubble and can thus escape unscathed, allowing astronomers to detect them.
“We expected that reionization bubbles from this era in cosmic history would be rare and hard to find,” said Sangeeta Malhotra, a collaborator at NASA GSFC, “so confirmation of this transition is important.” This “cosmic dawn”, the intermediate state between a neutral and an ionized Universe, is something that has been predicted. Such discoveries are made possible by the availability of powerful astronomical instruments that can probe the Universe in a way unimagined by past generations of astronomers.
 EGS, or the Extended Groth Strip, is a region imaged by HST in 2005; it corresponds to a narrow strip of the sky about the width of a finger held at arms length. There are at least 50,000 galaxies known within the strip.
This research will be presented in a forthcoming paper and is currently close to acceptance.
The research team is composed of:
V. Tilvi, School of Earth and Space Exploration, Arizona State University, Tempe, AZ; S. Malhotra, Astrophysics Science Division, Goddard Space Flight Center, Greenbelt, MD; J. E. Rhoads,Astrophysics Science Division, Goddard Space Flight Center, Greenbelt; A. Coughlin, Chandler-Gilbert Community College, Chandler, AZ; Z. Zheng, CAS Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Shangha, People’s Republic of China; S. L. Finkelstein,Department of Astronomy, University of Texas at Austin, Austin, TX; S. Veilleux, Department of Astronomy and Joint Space-Science Institute, University of Maryland, College Park, MD; B. Mobasher, Department of Physics and Astronomy, University of California, Riverside, CA; J. Wang, CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei, Anhui, People’s Republic of China; Rob Probst, NOAO, 950 N. Cherry Avenue, Tucson, AZ 85719.
NSF’s National Optical-Infrared Astronomy Research Laboratory, the US center for ground-based optical-infrared astronomy, operates the international Gemini Observatory (a facility of NSF, NRC–Canada, CONICYT–Chile, MCTI–Brazil, MCTIP–Argentina, and KASI–Republic of Korea), Kitt Peak National Observatory (KPNO), Cerro Tololo Inter-American Observatory (CTIO), the Community Science and Data Center (CSDC), and the Vera C. Rubin Observatory. It is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with NSF and is headquartered in Tucson, Arizona. The astronomical community is honored to have the opportunity to conduct astronomical research on Iolkam Du’ag (Kitt Peak) in Arizona, on Maunakea in Hawai’i, and on Cerro Tololo and Cerro Pachón in Chile. We recognize and acknowledge the very significant cultural role and reverence that these sites have to the Tohono O’odham Nation, to the Native Hawaiian community, and to the local communities in Chile, respectively.
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