11 September, 2017Scientific Paper
Astronomers found that active star formation upswells galaxies, like yeast helps bread rise. Using three powerful telescopes on the ground and in orbit, they observed galaxies from 11 billion years ago and found explosive formation of stars in the cores of galaxies. This suggests that galaxies can change their own shape without interaction with other galaxies.
“Massive elliptical galaxies are believed to be formed from collisions of disk galaxies,” said Ken-ichi Tadaki, the lead author of two research papers and a postdoctoral researcher at the National Astronomical Observatory of Japan (NAOJ). “But, it is uncertain whether all the elliptical galaxies have experienced galaxy collision. There may be an alternative path.”
Aiming to understand galactic metamorphosis, the international team explored distant galaxies 11 billion light-years away. Because it takes time for the light from distant objects to reach us, by observing galaxies 11 billion light-years away, the team can see what the Universe looked like 11 billion years ago, 3 billion years after the Big Bang. This corresponds the peak epoch of galaxy formation; the foundations of most galaxies were formed in this epoch.
Receiving faint light which has travelled 11 billion years is tough work. The team harnessed the power of three telescopes to anatomize the ancient galaxies. First, they used NAOJ’s 8.2-m Subaru Telescope in Hawai`i and picked out 25 galaxies in this epoch. Then they targeted the galaxies for observations with NASA/ESA’s Hubble Space Telescope (HST) and the Atacama Large Millimeter/submillimeter Array (ALMA). The astronomers used HST to capture the light from stars which tells us the “current” (as of when the light was emitted, 11 billion years ago) shape of the galaxies, while ALMA observed submillimeter waves from cold clouds of gas and dust, where new stars are being formed. By combining the two, we know the shapes of the galaxies 11 billion years ago and how they are evolving.
Thanks to their high resolution, HST and ALMA could illustrate the metamorphosis of the galaxies. With HST images the team found that a disk component dominates the galaxies. Meanwhile, the ALMA images show that there is a massive reservoir of gas and dust, the material of stars, so that stars are forming very actively. The star formation activity is so high that huge numbers of stars will be formed at the centers of the galaxies. This leads the astronomers to think that ultimately the galaxies will be dominated by the stellar bulge and become elliptical or lenticular galaxies.
“Here, we obtained firm evidence that dense galactic cores can be formed without galaxy collisions. They can also be formed by intense star formation in the heart of the galaxy.” said Tadaki. The team used the European Southern Observatory’s Very Large Telescope to observe the target galaxies and confirmed that there are no indications of massive galaxy collisions.
Almost 100 years ago, American astronomer Edwin Hubble invented the morphological classification scheme for galaxies. Since then, many astronomers have devoted considerable effort to understanding the origin of the variety in galaxy shapes. Utilizing the most advanced telescopes, modern astronomers have come one step closer to solving the mysteries of galaxies.
These observation results were published as Tadaki et al. “Bulge-forming Galaxies with an Extended Rotating Disk at z ~ 2” and “Rotating Starburst Cores in Massive Galaxies at z = 2.5” in the Astrophysical Journal Letters in January and May 2017, respectively.
The research team members are:
Ken-ichi Tadaki (Max-Planck-Institute for Extraterrestrial Physics [MPE]/National Astronomical Observatory of Japan [NAOJ]), Reinhard Genzel (MPE/University of California, Berkeley), Tadayuki Kodama (NAOJ/The Graduate University for Advanced Studies [SOKENDAI], Tohoku University), Stijn Wuyts (University of Bath), Emily Wisnioski (MPE), Natascha M. Foerster Schreiber (MPE), Andreas Burkert (MPE/Ludwig Maximilian University), Phillip Lang (MPE), Linda J. Tacconi (MPE), Dieter Lutz (MPE), Sirio Belli (MPE), Richard I. Davies (MPE), Bunyo Hatsukade (The University of Tokyo), Masao Hayashi (NAOJ), Rodrigo Herrera-Camus (MPE), Soh Ikarashi (University of Groningen), Shigeki Inoue (The University of Tokyo), Kotaro Kohno (The University of Tokyo), Yusei Koyama (NAOJ), J. Trevor Mendel (MPE / Ludwig Maximilian University), Kouichiro Nakanishi (NAOJ/SOKENDAI), Rhythm Shimakawa (SOEKNDAI/University of California), Tomoko L. Suzuki (SOEKNDAI/NAOJ), Yoichi Tamura (The University of Tokyo/Nagoya University), Ichi Tanaka (NAOJ), Hannah Uebler (MPE), Dave J. Wilman (MPE/ Ludwig Maximilian University), Erica J. Nelson (MPE), Magdalena Lippa (MPE)
This research was supported by the Japan Society for the Promotion of Science and the German Academic Exchange Service under the Japan-German Research Cooperative Program.
The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of the European Organisation for Astronomical Research in the Southern Hemisphere (ESO), the U.S. National Science Foundation (NSF) and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile. ALMA is funded by ESO on behalf of its Member States, by NSF in cooperation with the National Research Council of Canada (NRC) and the National Science Council of Taiwan (NSC) and by NINS in cooperation with the Academia Sinica (AS) in Taiwan and the Korea Astronomy and Space Science Institute (KASI).
ALMA construction and operations are led by ESO on behalf of its Member States; by the National Radio Astronomy Observatory (NRAO), managed by Associated Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical Observatory of Japan (NAOJ) on behalf of East Asia. The Joint ALMA Observatory (JAO) provides the unified leadership and management of the construction, commissioning and operation of ALMA.