Figure 1: Pseudo-color composite image of PKS 1138-262 region, derived from Hubble Space Telescope's ACS/WFC data archive (F814W and F475W). This region is one of the target protoclusters observed by MOIRCS on Subaru Telescope. (Credit: NAOJ/HST)
Figure 2: Mass-growth history expected of massive cluster of galaxies that have about 10^15 solar masses present day. Red spots are from this study. Black and grayer are for other massive cluster of galaxies, studied by the author's team and other research teams, respectively. (Credit: NAOJ)
Figure 3: Plot of stellar mass of the galaxies versus metallicity of gas in them. Gray and pale blue curves are for the present-day (nearby) galaxies and field galaxies at 11 billion years ago, respectively. Red is the current study about the proto-cluster of galaxies. The galaxies in the proto-clusters clearly show higher metallicity compared with the ones in the general fields at about the same time of the history in the universe. (Credit: NAOJ)
Figure 4: Illustrations of the metal enrichment processes (chemical evolution) in the field galaxies and the proto-cluster galaxies. Left (figure 4a) is for the galaxies in the general fields while the middle and the right (figures 4b and 4c, respectively) show their model that explain the unique enrichment processes of the heavy elements in the galaxies in the proto-clusters. (Credit: NAOJ)
Figure 2: Mass-growth history expected of massive cluster of galaxies that have about 10^15 solar masses present day. Red spots are from this study. Black and grayer are for other massive cluster of galaxies, studied by the author's team and other research teams, respectively. (Credit: NAOJ)
Figure 3: Plot of stellar mass of the galaxies versus metallicity of gas in them. Gray and pale blue curves are for the present-day (nearby) galaxies and field galaxies at 11 billion years ago, respectively. Red is the current study about the proto-cluster of galaxies. The galaxies in the proto-clusters clearly show higher metallicity compared with the ones in the general fields at about the same time of the history in the universe. (Credit: NAOJ)
Figure 4: Illustrations of the metal enrichment processes (chemical evolution) in the field galaxies and the proto-cluster galaxies. Left (figure 4a) is for the galaxies in the general fields while the middle and the right (figures 4b and 4c, respectively) show their model that explain the unique enrichment processes of the heavy elements in the galaxies in the proto-clusters. (Credit: NAOJ)
Ongoing studies of distant galaxy protoclusters using the Multi-Object
Infrared Camera and Spectrograph (MOIRCS) instrument on the Subaru
Telescope is giving astronomers a closer look at the characteristics of
star-forming regions in galaxies in the early universe. A team of
astronomers from the National Astronomical Observatory of Japan (NAOJ)
and SOKENDAI (Graduate University of Advanced Studies, Japan) are
tracking velocity structures and gaseous metallicities in galaxies in
two protoclusters located in the direction of the constellation Serpens.
These appear around the radio galaxies PKS 1138-262 (at a redshift of
2.2, Figure 1)
and USS 1558-003 (at a redshift of 2.5). The clusters appear as they
would have looked 11 billion years ago, and the team concluded that they
are in the process of cluster formation that has led to present-day
galaxy clusters.
The MOIRCS near-infrared spectrograph is very
effective for studies focused on the distant, early universe because
strong emission lines from star-forming galaxies are redshifted from the
optical to the near-infrared regime. This gives astronomers unique
insights into these activities. (Note 1)
Based on the MOIRCS data, the team estimated that both protoclusters have a weight of about 10^14 solar masses (Figure 2).
These follow the typical mass growth history of the today's most
massive clusters, such as the 'Coma Cluster.' That makes the two
protoclusters ideal laboratories for exploring early phasesof galaxy
formation in a unique clustered environment.
The metallicity of the gases in the protocluster galaxies was studied
using multiple spectral lines emitted from them. The result shows their
gaseous metallicities are chemically enriched compared with those of
galaxies in the general fields (Figure 3).
Metals (elements heavier than hydrogen and helium) are created in the
interiors of stars as they evolve and then released into surrounding gas
through supernova explosions or stellar winds (often referred to as
chemical evolution; Figure 4a).
The difference in gaseous metallicity between
protoclusters and general fields suggests that star-formation histories
and/or gas inflow/outflow processes should be different in the
protocluster regions. The result also suggests that galaxy formation has
already been influenced by environmental conditions in the era that
star-formation activities are the most active across the universe. This
would be an early phase of strong environmental effects seen in the
present galaxy clusters.
In order to explain the metallicity excess in the
protoclusters, the team members focused attention on the environmental
effects of inflow and outflow mechanism on the galaxy formation process.
Recent works report that inflow and outflow activities were most
significant eleven billion years ago (at redshift ~2), and were about a
hundred times more active relative to those in the local universe.
Clusters of galaxies are large self-gravitating
systems in which galaxies and ionized gas are bound by massive amounts
of dark matter. In such unique, dense environments, galaxies move at a
speed of about 1000 kilometers per second. Due to this high speed, the
galaxies are exposed to high pressure from intercluster medium. As a
result, the outer regions with relatively poor metallicity are stripped.
It is like the strong air resistance of air a bicycle rider
experiences. In this case, the gaseous metallicities become higher
because the chemical enrichment process takes place mainly in metal-rich
central regions (Figure 4b).
Another possibility is that the surrounding high-pressure,
inter-cluster medium prevents outflowing gas from escaping from the
galaxies (Figure 4c). This also results in higher gaseous metallicities of the cluster galaxies.
The research team concludes that the metallicity
excess in the protocluster regions results from unique phenomena
occurring in the cluster environment. The PI of this research, Mr.
Rhythm Shimakawa of NAOJ and SOKENDAI (Note 2),
is determined to continue studying the detailed physical properties of
individual forming galaxies in the protoclusters to find clear evidence
that proves this hypothesis.
This article is based on results from two research papers published in the Monthly Notices of the Royal Astronomical Society:
Rhythm Shimakawa, Tadayuki Kodama, Ken-ichi Tadaki,
Ichi Tanaka, Masao Hayashi and Yusei Koyama, "Identification of the
progenitors of rich clusters and member galaxies in rapid formation at z
> 2", Volume 441, Issue 1, p.L1-L5, published in June 11, 2014,
and
Rhythm Shimakawa, Tadayuki Kodama, Ken-ichi Tadaki, Masao Hayashi, Yusei Koyama, Ichi Tanaka "An early phase of environmental effects on galaxy properties unveiled by near-infrared spectroscopy of protocluster galaxies at z>2", Volume 448, Issue 1, p.666-680, published in March 21, 2015.
and
Rhythm Shimakawa, Tadayuki Kodama, Ken-ichi Tadaki, Masao Hayashi, Yusei Koyama, Ichi Tanaka "An early phase of environmental effects on galaxy properties unveiled by near-infrared spectroscopy of protocluster galaxies at z>2", Volume 448, Issue 1, p.666-680, published in March 21, 2015.
This research is supported in part by a Grant-in-Aid
for the Scientific Research (Nos. 21340045 and 24244015) by the Japanese
Ministry of Education, Culture, Sports, Science and Technology.
Authors:
- Rhythm Shimakawa (Subaru Telescope, National Astronomical Observatory of Japan [NAOJ]/SOKENDAI(Graduate University for Advanced Studies))
- Tadayuki Kodama (Optical and Infrared Astronomy Division, NAOJ/SOKENDAI)
- Ichi Tanaka (Subaru Telescope, NAOJ)
- Kenichi Tadaki (Max-Planck-Institute fur Extraterrestrische Physic, Germany)
- Masao Hayashi (Optical and Infrared Astronomy Division, NAOJ)
- Yusei Koyama (Institute of Space Astronomical Science, Japan Aerospace Exploration Agency)
Notes:
- See the Web release by M. Hayashi, "Discovery of an Ancient Celestial City Undergoing Rapid Growth: A Young Protocluster of Active Star-Forming Galaxies".
- Mr. Rhythm Shimakawa received the first "SOKENDAI Future Scientist Award" for his research "Environmental effects on galaxy formation: When and how did spiral and elliptical galaxies diverge?", which includes the two papers referred in this article.
Source: Subaru Telescope