The GALAH survey: chemical homogeneity of the Orion complex

Kos, Janez and Bland-Hawthorn, Joss and Buder, Sven and Nordlander, Thomas and Spina, Lorenzo and Beeson, Kevin L. and Lind, Karin and Asplund, Martin and Freeman, Ken and Hayden, Michael R. and Lewis, Geraint F. and Martell, Sarah L. and Sharma, Sanjib and de Silva, Gayandhi and Simpson, Jefferey D. and Zucker, Daniel B. and Zwitter, Tomaz and Cotar, Klemen and Horner, Jonti and Ting, Yuan-Sen and Traven, Gregor (2021) The GALAH survey: chemical homogeneity of the Orion complex. Monthly Notices of the Royal Astronomical Society. ISSN 0035-8711

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Abstract

Due to its proximity, the Orion star forming region is often used as a proxy to study processes related to star formation and to observe young stars in the environment they were born in. With the release of Gaia DR2, the distance measurements to the Orion complex are now good enough that the three dimensional structure of the complex can be explored. Here we test the hypothesis that, due to non-trivial structure and dynamics, and age spread in the Orion complex, the chemical enrichment of youngest stars by early core-collapse supernovae can be observed. We obtained spectra of 794 stars of the Orion complex with the HERMES spectrograph at the Anglo Australian telescope as a part of the GALAH and GALAH-related surveys. We use the spectra of ~300 stars to derive precise atmospheric parameters and chemical abundances of 25 elements for 15 stellar clusters in the Orion complex. We demonstrate that the Orion complex is chemically homogeneous and that there was no self-pollution of young clusters by core-collapse supernovae from older clusters; with a precision of 0.02 dex in relative alpha-elements abundance and 0.06 dex in oxygen abundance we would have been able to detect pollution from a single supernova, given a fortunate location of the SN and favourable conditions for ISM mixing. We estimate that the supernova rate in the Orion complex was very low, possibly producing no supernova by the time the youngest stars of the observed population formed (from around 21 to 8 Myr ago).


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Item Type: Article (Commonwealth Reporting Category C)
Refereed: Yes
Item Status: Live Archive
Additional Information: © 2021 The Author(s). Published online: 28 June 2021. Publisher's Accepted version deposited in accordance with the copyright policy of the publisher.
Faculty/School / Institute/Centre: Current - Institute for Advanced Engineering and Space Sciences - Centre for Astrophysics (1 Aug 2018 -)
Faculty/School / Institute/Centre: Current - Institute for Advanced Engineering and Space Sciences - Centre for Astrophysics (1 Aug 2018 -)
Date Deposited: 22 Jul 2021 01:24
Last Modified: 27 Jul 2021 00:20
Uncontrolled Keywords: astrochemistry; surveys; stars; abundances; formation; pre-main-sequence; open clusters and associations; astrophysics; galaxies
Fields of Research (2008): 02 Physical Sciences > 0201 Astronomical and Space Sciences > 020110 Stellar Astronomy and Planetary Systems
Fields of Research (2020): 51 PHYSICAL SCIENCES > 5101 Astronomical sciences > 510109 Stellar astronomy and planetary systems
Socio-Economic Objectives (2008): E Expanding Knowledge > 97 Expanding Knowledge > 970102 Expanding Knowledge in the Physical Sciences
Socio-Economic Objectives (2020): 28 EXPANDING KNOWLEDGE > 2801 Expanding knowledge > 280120 Expanding knowledge in the physical sciences
Identification Number or DOI: https://doi.org/10.1093/mnras/stab1767
URI: http://eprints.usq.edu.au/id/eprint/42818

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