From IAC-The Institute of Astrophysics of the Canary Islands [Instituto de Astrofísica de Canarias] (ES) : “Astronomers find Milky Way analogue galaxy in the early universe”

Instituto de Astrofísica de Andalucía

From IAC-The Institute of Astrophysics of the Canary Islands [Instituto de Astrofísica de Canarias] (ES)


Zoom-in on the Cosmic Seahorse in visual and near infrared light. The foreground giant elliptical galaxy, at the center of a galaxy cluster, magnifies and distorts the distant light coming from the strongly lensed galaxy. Credit: NASA/ESA Hubble.

National Aeronautics and Space Administration(US)/European Space Agency [Agence spatiale européenne] [Europäische Weltraumorganisation](EU) Hubble Space Telescope.

An international team, including researchers from the Instituto de Astrofísica de Canarias (IAC), used combined data from different radio telescopes located in Spain to probe the mode of star formation in a galaxy when the universe had less than 30% of its current age. They revealed that the properties of the molecular gas reservoir are similar to the one of our own Galaxy, unseen up to now in the distant universe. The paper is published in The Astrophysical Journal Letters.

A major question in the study of galaxies is on the mode of star formation, how efficient the conversion of cold gas into stars is. Up to now, galaxies in the early universe seem to form stars in a different manner than observed in our own Galaxy which is puzzling. To shed light onto this question, the cold molecular gas, the fuel for the formation of stars, gets observed with radio telescopes.

Due to the physical properties of the molecular hydrogen gas (H2), it cannot be observed directly in the radio regime but it can traced via the carbon monoxide molecule (CO). And that is what the team led by Nikolaus Sulzenauer, a PhD student at The MPG Institute for Radio Astronomy[MPG Institut für Radioastronomie](DE) has done.

First, the researchers selected a galaxy whose brightness is boosted through gravitational lensing by an intervening cluster of galaxies. They then searched for archival data of infrared space missions in combination with the Hubble Space Telescope imaging.

“The discovered galaxy is strongly lensed by a factor of about 10 and thus its morphology is distorted resembling a seahorse.

Gravitational Lensing Gravitational Lensing National Aeronautics Space Agency (US) and European Space Agency [Agence spatiale européenne][Europäische Weltraumorganisation](EU).

Therefore its nickname is “the Cosmic Seahorse” explains Sulzenauer, who carried out this study as a master’s thesis at The University of Vienna [Universität Wien](AT) under the supervision of IAC researcher Helmut Dannerbauer who is also co-author of the paper that is published in The Astrophysical Journal Letters.

Detail of the “cosmic seahorse”, a galaxy modified by gravitational lensing. Illustration: Carla Nicolin Schoder (Univ. Vienna)

The researcher revealed the distance of this galaxy, the light travelled 9.6 billion years, through observations of the carbon monoxide lines with the 30 m radio telescope of the Instituto de Radioastronomía Milimétrica (IRAM) located in the Sierra Nevada.

IRAM 30m Radio telescope in Spain.

Together with observations of the Yebes 40 m radio telescope located at Yebes, 50 km north-east of Madrid and operated by the Instituto Geográfico Nacional (IGN), the physical properties of the fuel of star formation through the observations of several molecular gas lines could be derived as well.

Yebes 40 m radio telescope located at Yebes, 50 km north-east of Madrid.

“That it is the most distant galaxy detected with the Yebes 40 m radio telescope up to now” notes Dannerbauer, who also highlights the advantage that the method used in the research has brought to these radio telescopes: “The gravitational lensing virtually transforms the IRAM and Yebes telescopes into radio telescopes with sizes of single dishes of 300 resp. 400 m, impossible to construct.”

Through the analysis of the cold molecular gas, the researchers found the presence of previously unseen star-formation mechanism at cosmic noon, the peak epoch of star formation and black hole activity of the universe. “Our research has shown that this is a so-called main-sequence galaxy with slowly evolving star formation at the epoch of maximum star formation in the Universe” adds Bodo Ziegler from the University of Vienna and co-author of the article.

“This seems to be the missing link between systems with high and low star formation rate such as the Cosmic Seahorse” explains Anastasio Díaz Sánchez of The Polytechnic University of Cartagena[Universidad Politécnica de Cartagena](ES) who also participated in the study. Likewise, Susana Iglesias Groth, IAC researcher and co-author of the article, emphasises the relevance of this discovery considering the difficulty of studying this type of galaxy: “Without the gravitational lensing it would have been impossible to detect this galaxy, with calm star formation activity, with these large radio telescopes.”

See the full article here .


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IAC-The Institute of Astrophysics of the Canary Islands [Instituto de Astrofísica de Canarias] (ES) operates two astronomical observatories in the Canary Islands:

Roque de los Muchachos Observatory on La Palma
Teide Observatory on Tenerife.

The Instituto de Astrofísica the headquarters, which is in La Laguna (Tenerife).

Observatorio del Roque de los Muchachos at La Palma (ES) at an altitude of 2400m.

The seeing statistics at ORM make it the second-best location for optical and infrared astronomy in the Northern Hemisphere, after Mauna Kea Observatory Hawaii (US).

Maunakea Observatories Hawai’i (US) altitude 4,213 m (13,822 ft).

The site also has some of the most extensive astronomical facilities in the Northern Hemisphere; its fleet of telescopes includes the 10.4 m Gran Telescopio Canarias, the world’s largest single-aperture optical telescope as of July 2009, the William Herschel Telescope (second largest in Europe), and the adaptive optics corrected Swedish 1-m Solar Telescope.

Gran Telescopio Canarias [Instituto de Astrofísica de Canarias ](ES) sited on a volcanic peak 2,267 metres (7,438 ft) above sea level.

Isaac Newton Group 4.2 meter William Herschel Telescope at Roque de los Muchachos Observatory on La Palma in the Canary Islands(ES), 2,396 m (7,861 ft).

The Swedish 1m Solar Telescope SST at the Roque de los Muchachos observatory on La Palma Spain, Altitude 2,360 m (7,740 ft).

The observatory was established in 1985, after 15 years of international work and cooperation of several countries with the Spanish island hosting many telescopes from Britain, The Netherlands, Spain, and other countries. The island provided better seeing conditions for the telescopes that had been moved to Herstmonceux by the Royal Greenwich Observatory, including the 98 inch aperture Isaac Newton Telescope (the largest reflector in Europe at that time). When it was moved to the island it was upgraded to a 100-inch (2.54 meter), and many even larger telescopes from various nations would be hosted there.

Tiede Observatory, Tenerife, Canary Islands (ES)

Teide Observatory [Observatorio del Teide], IAU code 954, is an astronomical observatory on Mount Teide at 2,390 metres (7,840 ft), located on Tenerife, Spain. It has been operated by the Instituto de Astrofísica de Canarias since its inauguration in 1964. It became one of the first major international observatories, attracting telescopes from different countries around the world because of the good astronomical seeing conditions. Later the emphasis for optical telescopes shifted more towards Roque de los Muchachos Observatory on La Palma.