{"id":11765,"date":"2021-02-22T09:00:42","date_gmt":"2021-02-22T19:00:42","guid":{"rendered":"http:\/\/www.eaobservatory.org\/jcmt\/?p=11765"},"modified":"2021-02-26T13:11:39","modified_gmt":"2021-02-26T23:11:39","slug":"jcmt-alma-stellar-nurseries-orion","status":"publish","type":"post","link":"https:\/\/www.eaobservatory.org\/jcmt\/2021\/02\/jcmt-alma-stellar-nurseries-orion\/","title":{"rendered":"JCMT and ALMA: Hunting for stellar nurseries in Orion"},"content":{"rendered":"

Stars are known to form in so-called \u201cmolecular clouds\u201d; collections of cold gas and dust in the space between stars. These stellar nurseries can contain a number of dense clumps of gas and dust called \u201cprestellar cores”. Research has suggested that these cores are expected to exhibit concentrated structures within them – the \u201cseeds\u201d of new stars right at the cusp of being born.<\/p>\n

Strong efforts by astronomers have been made to find such \u201cseeds\u201d of stars inside prestellar cores in the past, but mostly in vain. It was difficult to catch such seeds in action perhaps because they are short-lived, but also due to the inherent difficulties in observing such dense regions and at such small scales. Despite the challenges, Dipen Sahu, at the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA), Taiwan, and lead author of this study stated that \u201cdespite the challenges it is very important to understand when and how such stellar embryo(s) come to live\u201d noting that \u201cit is this critical early stage that is important to observe as we understand how these early stages shape the stellar offspring. We would like to know how stellar systems are formed, but we need to study them near their birth to fully understand the process.\u201d<\/p>\n

We would like to know how stellar systems are formed, but we need to find them near their birth to understand the process.<\/i><\/strong><\/span><\/p>\n

One of the closest, brightest and most well known stellar nurseries can be found in the constellation of Orion also known as the Ka Hei-Hei O N\u0101 Keiki (which refers to a children’s string game similar to the cat\u2019s cradle) in Hawaiian. The international team, including astronomers from Taiwan, China, Japan, and Korea, first started out to uncover cold and dense cores in the Orion Molecular Cloud. As dust in the cores absorbs light and blocks the view at the optical wavelengths, astronomers make use of “light” emitted by the dust inside the dense cores at submillimeter wavelengths, obtained using such telescopes as the James Clark Maxwell Telescope (JCMT) situated on the slopes of Maunakea in Hawaii.<\/p>\n

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Core \u201cG205.46-14.56M3\u201d located in the Orion Molecular Cloud shows signs of multiple small blobs inside. Top right insert: SCUBA-2 image of G2-5.46-14.56M3 as observed by the JCMT, Hawaii. Bottom left insert: ALMA resolves the newly forming stars within. The Orion Constellation is also known as the Ka Hei-Hei O N\u0101 Keiki (\u201cthe cat\u2019s cradle\u201d) in Hawaiian. Credit: ASIAA\/Wei-Hao Wang\/ALMA (ESO\/NAOJ\/NRAO)\/Tie Lie\/Sahu et al. <\/strong><\/p><\/div>\n

\u201cThe JCMT continues to play a pivotal role in locating these cores!\u201d, says Tie Liu at Shanghai Astronomical Observatory, co-author of this study and the principal investigator of the ALMA observation program, \u201cthe JCMT is critical in that it gives us the speed to hunt around these stellar nurseries with the sensitivity needed to find these faint regions of cold and dense gas\u201d.<\/p>\n

With JCMT providing the team with stellar nursery candidates, the team turned to the largest telescope on the ground to date, the Atacama Large Millimeter and submillimeter Array (ALMA) located in the high desert in northern Chile. The observations carried out with ALMA in late 2018 to early 2019 unveil to the team five cores with\u00a0 a very concentrated gas and dust distribution at a scale of a 1000 AU. Toward one core named \u201cG205.46-14.56M3\u201d in particular, the image shows signs of multiple small peak structures inside. These peaks are estimated to harbor a high density of cold gas that has never been seen before and their significant mass makes astronomers think that they are very likely to form a binary star system in the future. It is known that a large fraction of Sun-like stars are in binary or multiple stellar systems. Sheng-Yuan Liu at ASIAA, co-author of this study stated \u201cALMA provides us with unprecedented sensitivity and angular resolution so that we can see faint sources with truly sharp images. Finding twins or triplets should be common in stellar nurseries but it is remarkable to actually obtain the image like seeing inside an egg with two yolks!\u201d<\/p>\n

Finding twins or triplets should be common in stellar nurseries but it is remarkable to actually obtain the image like seeing inside an egg with two yolks!<\/em><\/strong><\/span><\/p>\n

It remains unclear what leads to the sub-structures we see in the core of G205.46-14.56M3. The substructures are likely a complicated interplay between the gas motion, gravity, and magnetic fields that are threading through the gas. The observed emission from the dust only tells us how gas and dust are distributed. Understanding how the gas is moving and how magnetic fields are distributed inside such cores would allow astronomers to further pinpoint the decisive process.<\/p>\n

\u201cDetecting such a handful of stellar seeds is just the beginning and the JCMT has proven to be a great tool for uncovering these nurseries. I am excited to see what new discoveries we will make when we combine the power of both JCMT and future followup studies with ALMA\u201d, says Dipen Sahu.<\/p>\n

The publication<\/strong><\/h3>\n

This work was published: \u201cALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Detection of Extremely High-density Compact Structure of Prestellar Cores and Multiple Substructures Within<\/a>\u201d by Dipen Sahu et al. in the Astrophysical Journal Letters.<\/p>\n

The team is composed of Dipen Sahu (Academia Sinica Institute of Astronomy and Astrophysics), Sheng-Yuan Liu (Academia Sinica Institute of Astronomy and Astrophysics), Tie Liu (Shanghai Astronomical Observatory, Chinese Academy of Sciences), Neal J. Evans II (Department of Astronomy The University of Texas at Austin), Naomi Hirano (Academia Sinica Institute of Astronomy and Astrophysics), Ken’ichi Tatematsu (Nobeyama Radio Observatory, National Astronomical Observatory of Japan, National Institutes of Natural Sciences), Chin-Fei Lee(Academia Sinica Institute of Astronomy and Astrophysics), Kee-Tae Kim (Korea Astronomy and Space Science Institute), Somnath Dutta (Academia Sinica Institute of Astronomy and Astrophysics), Dana Alina (Department of Physics, School of Sciences and Humanities, Nazarbayev University)<\/p>\n

Contact Information<\/b><\/h3>\n

Dr. Sheng-Yuan Liu<\/strong>
\nAcademia Sinica Institute of Astronomy and Astrophysics
\nASIAA, Taiwan
\nEmail: syliu@asiaa.sinica.edu.tw<\/p>\n

Dr. Jessica Dempsey<\/strong>
\nJames Clerk Maxwell Telescope
\nEast Asian Observatory, Hawaii, USA
\nEmail: \u200bj.dempsey@eaobservatory.org<\/p>\n

Media Releases:<\/h3>\n