--- _id: '11600' abstract: - lang: eng text: The Sun’s surface hosts varying magnetic activities and rotation rates (from equator to pole), and unique solar weather. Now, a combination of ground and space observations has unveiled a previously undetected magnetized plasma current. article_processing_charge: No article_type: letter_note author: - first_name: Lisa Annabelle full_name: Bugnet, Lisa Annabelle id: d9edb345-f866-11ec-9b37-d119b5234501 last_name: Bugnet orcid: 0000-0003-0142-4000 citation: ama: Bugnet LA. Hidden currents at the Sun’s surface. Nature Astronomy. 2022;6:631-632. doi:10.1038/s41550-022-01683-2 apa: Bugnet, L. A. (2022). Hidden currents at the Sun’s surface. Nature Astronomy. Springer Nature. https://doi.org/10.1038/s41550-022-01683-2 chicago: Bugnet, Lisa Annabelle. “Hidden Currents at the Sun’s Surface.” Nature Astronomy. Springer Nature, 2022. https://doi.org/10.1038/s41550-022-01683-2. ieee: L. A. Bugnet, “Hidden currents at the Sun’s surface,” Nature Astronomy, vol. 6. Springer Nature, pp. 631–632, 2022. ista: Bugnet LA. 2022. Hidden currents at the Sun’s surface. Nature Astronomy. 6, 631–632. mla: Bugnet, Lisa Annabelle. “Hidden Currents at the Sun’s Surface.” Nature Astronomy, vol. 6, Springer Nature, 2022, pp. 631–32, doi:10.1038/s41550-022-01683-2. short: L.A. Bugnet, Nature Astronomy 6 (2022) 631–632. date_created: 2022-07-18T09:34:37Z date_published: 2022-05-18T00:00:00Z date_updated: 2022-08-19T09:52:21Z day: '18' doi: 10.1038/s41550-022-01683-2 extern: '1' intvolume: ' 6' keyword: - Astronomy and Astrophysics language: - iso: eng month: '05' oa_version: None page: 631-632 publication: Nature Astronomy publication_identifier: eissn: - 2397-3366 publication_status: published publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: Hidden currents at the Sun’s surface type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 6 year: '2022' ... --- _id: '11585' abstract: - lang: eng text: "Observations show that star-forming galaxies reside on a tight three-dimensional plane between mass, gas-phase metallicity and star formation rate (SFR), which can be explained by the interplay between metal-poor gas inflows, SFR and outflows. However, different metals are released on different time-scales, which may affect the slope of this relation. Here, we use central, star-forming galaxies with Mstar = 109.0−10.5 M\f from the EAGLE hydrodynamical simulation to examine three-dimensional relations between mass, SFR and chemical enrichment using absolute and relative C, N, O and Fe abundances. We show that the scatter is smaller when gas-phase α-enhancement is used rather than metallicity. A similar plane also exists for stellar α-enhancement, implying that present-day specific SFRs are correlated with long time-scale star formation histories. Between z = 0 and 1, the α-enhancement plane is even more insensitive to redshift than the plane using metallicity. However, it evolves at z > 1 due to lagging iron yields. At fixed mass, galaxies with higher SFRs have star formation histories shifted toward late times, are more α-enhanced and this α-enhancement increases with redshift as observed. These findings suggest that relations between physical properties inferred from observations may be affected by systematic variations in α-enhancements." acknowledgement: We thank the anonymous referee for their constructive comments. JM acknowledges the support of a Huygens PhD fellowship from Leiden University. We thank Jarle Brinchmann, Rob Crain and David Sobral for discussions. We acknowledge the use of the Topcat software (Taylor 2013) for assisting in rapid exploration of multi-dimensional datasets and the use of Python and its numpy, matplotlib and pandas packages. article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Jorryt J full_name: Matthee, Jorryt J id: 7439a258-f3c0-11ec-9501-9df22fe06720 last_name: Matthee orcid: 0000-0003-2871-127X citation: ama: Matthee JJ. Differences in galaxy colours are not just about the mass. Nature Astronomy. 2021;5:984-985. doi:10.1038/s41550-021-01415-y apa: Matthee, J. J. (2021). Differences in galaxy colours are not just about the mass. Nature Astronomy. Springer Nature. https://doi.org/10.1038/s41550-021-01415-y chicago: Matthee, Jorryt J. “Differences in Galaxy Colours Are Not Just about the Mass.” Nature Astronomy. Springer Nature, 2021. https://doi.org/10.1038/s41550-021-01415-y. ieee: J. J. Matthee, “Differences in galaxy colours are not just about the mass,” Nature Astronomy, vol. 5. Springer Nature, pp. 984–985, 2021. ista: Matthee JJ. 2021. Differences in galaxy colours are not just about the mass. Nature Astronomy. 5, 984–985. mla: Matthee, Jorryt J. “Differences in Galaxy Colours Are Not Just about the Mass.” Nature Astronomy, vol. 5, Springer Nature, 2021, pp. 984–85, doi:10.1038/s41550-021-01415-y. short: J.J. Matthee, Nature Astronomy 5 (2021) 984–985. date_created: 2022-07-14T13:13:39Z date_published: 2021-07-05T00:00:00Z date_updated: 2022-08-19T08:37:58Z day: '05' doi: 10.1038/s41550-021-01415-y extern: '1' external_id: arxiv: - '1802.06786' intvolume: ' 5' keyword: - Astronomy and Astrophysics - galaxies - formation - galaxies - evolution - galaxies - star formation - galaxies - abundances language: - iso: eng main_file_link: - open_access: '1' url: https://arxiv.org/abs/1802.06786 month: '07' oa: 1 oa_version: Preprint page: 984-985 publication: Nature Astronomy publication_identifier: eissn: - 2397-3366 publication_status: published publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: Differences in galaxy colours are not just about the mass type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 5 year: '2021' ... --- _id: '11611' abstract: - lang: eng text: Over the course of its history, the Milky Way has ingested multiple smaller satellite galaxies1. Although these accreted stellar populations can be forensically identified as kinematically distinct structures within the Galaxy, it is difficult in general to date precisely the age at which any one merger occurred. Recent results have revealed a population of stars that were accreted via the collision of a dwarf galaxy, called Gaia–Enceladus1, leading to substantial pollution of the chemical and dynamical properties of the Milky Way. Here we identify the very bright, naked-eye star ν Indi as an indicator of the age of the early in situ population of the Galaxy. We combine asteroseismic, spectroscopic, astrometric and kinematic observations to show that this metal-poor, alpha-element-rich star was an indigenous member of the halo, and we measure its age to be 11.0±0.7 (stat) ±0.8 (sys) billion years. The star bears hallmarks consistent with having been kinematically heated by the Gaia–Enceladus collision. Its age implies that the earliest the merger could have begun was 11.6 and 13.2 billion years ago, at 68% and 95% confidence, respectively. Computations based on hierarchical cosmological models slightly reduce the above limits. acknowledgement: This paper includes data collected by the TESS mission, which are publicly available from the Mikulski Archive for Space Telescopes (MAST). Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center for the production of the SPOC data products. W.J.C. acknowledges support from the UK Science and Technology Facilities Council (STFC) and UK Space Agency. Funding for the Stellar Astrophysics Centre is provided by The Danish National Research Foundation (grant agreement number DNRF106). This research was partially conducted during the Exostar19 programme at the Kavli Institute for Theoretical Physics at UC Santa Barbara, which was supported in part by the National Science Foundation under grant number NSF PHY-1748958. A.M., J.T.M., F.V. and J.M. acknowledge support from the ERC Consolidator Grant funding scheme (project ASTEROCHRONOMETRY, grant agreement number 772293). F.V. acknowledges the support of a Fellowship from the Center for Cosmology and AstroParticle Physics at The Ohio State University. W.H.B. and M.B.N. acknowledge support from the UK Space Agency. K.J.B. is supported by the National Science Foundation under award AST-1903828. M.B.N. acknowledges partial support from the NYU Abu Dhabi Center for Space Science under grant number G1502. A.M.S. is partially supported by the Spanish Government (ESP2017-82674-R) and Generalitat de Catalunya (2017-SGR-1131). T.M. acknowledges financial support from Belspo for contract PRODEX PLATO. H.K. acknowledges support from the European Social Fund via the Lithuanian Science Council grant number 09.3.3-LMT-K-712-01-0103. S.B. acknowledges support from NSF grant AST-1514676 and NASA grant 80NSSC19K0374. V.S.A. acknowledges support from the Independent Research Fund Denmark (research grant 7027-00096B). D.H. acknowledges support by the National Aeronautics and Space Administration (80NSSC18K1585, 80NSSC19K0379) awarded through the TESS Guest Investigator Program and by the National Science Foundation (AST-1717000). T.S.M. acknowledges support from a visiting fellowship at the Max Planck Institute for Solar System Research. Computational resources were provided through XSEDE allocation TG-AST090107. D.L.B. acknowledges support from NASA under grant NNX16AB76G. T.L.C. acknowledges support from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement number 792848 (PULSATION). This work was supported by FCT/MCTES through national funds (PIDDAC) by means of grant UID/FIS/04434/2019. K.J.B., S.H., J.S.K. and N.T. are supported by the European Research Council under the European Community’s Seventh Framework Programme (FP7/2007-2013)/ERC grant agreement number 338251 (StellarAges). E.C. is funded by the European Union’s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie grant agreement number 664931. L.G.-C. acknowledges support from the MINECO FPI-SO doctoral research project SEV-2015-0548-17-2 and predoctoral contract BES-2017-082610. P.G. is supported by the German space agency (Deutsches Zentrum für Luft- und Raumfahrt) under PLATO data grant 50OO1501. R.K. acknowledges support from the UK Science and Technology Facilities Council (STFC), under consolidated grant ST/L000733/1. M.S.L. is supported by the Carlsberg Foundation (grant agreement number CF17-076). Z.C.O., S.O. and M.Y. acknowledge support from the Scientific and Technological Research Council of Turkey (TÜBİTAK:118F352). S.M. acknowledges support from the Spanish ministry through the Ramon y Cajal fellowship number RYC-2015-17697. T.S.R. acknowledges financial support from Premiale 2015 MITiC (PI B. Garilli). R.Sz. acknowledges the support from NKFIH grant project No. K-115709, and the Lendület program of the Hungarian Academy of Science (project number 2018-7/2019). J.T. acknowledges support was provided by NASA through the NASA Hubble Fellowship grant number 51424 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. This work was supported by FEDER through COMPETE2020 (POCI-01-0145-FEDER-030389. A.M.B. acknowledges funding from the European Union’s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie grant agreement No 749962 (project THOT). A.M. and P.R. acknowledge the support of the Government of India, Department of Atomic Energy, under Project No. 12-R&D-TFR-6.04-0600. K.J.B. is an NSF Astronomy and Astrophysics Postdoctoral Fellow and DIRAC Fellow. article_processing_charge: No article_type: letter_note arxiv: 1 author: - first_name: William J. full_name: Chaplin, William J. last_name: Chaplin - first_name: Aldo M. full_name: Serenelli, Aldo M. last_name: Serenelli - first_name: Andrea full_name: Miglio, Andrea last_name: Miglio - first_name: Thierry full_name: Morel, Thierry last_name: Morel - first_name: J. Ted full_name: Mackereth, J. Ted last_name: Mackereth - first_name: Fiorenzo full_name: Vincenzo, Fiorenzo last_name: Vincenzo - first_name: Hans full_name: Kjeldsen, Hans last_name: Kjeldsen - first_name: Sarbani full_name: Basu, Sarbani last_name: Basu - first_name: Warrick H. full_name: Ball, Warrick H. last_name: Ball - first_name: Amalie full_name: Stokholm, Amalie last_name: Stokholm - first_name: Kuldeep full_name: Verma, Kuldeep last_name: Verma - first_name: Jakob Rørsted full_name: Mosumgaard, Jakob Rørsted last_name: Mosumgaard - first_name: Victor full_name: Silva Aguirre, Victor last_name: Silva Aguirre - first_name: Anwesh full_name: Mazumdar, Anwesh last_name: Mazumdar - first_name: Pritesh full_name: Ranadive, Pritesh last_name: Ranadive - first_name: H. M. full_name: Antia, H. M. last_name: Antia - first_name: Yveline full_name: Lebreton, Yveline last_name: Lebreton - first_name: Joel full_name: Ong, Joel last_name: Ong - first_name: Thierry full_name: Appourchaux, Thierry last_name: Appourchaux - first_name: Timothy R. full_name: Bedding, Timothy R. last_name: Bedding - first_name: Jørgen full_name: Christensen-Dalsgaard, Jørgen last_name: Christensen-Dalsgaard - first_name: Orlagh full_name: Creevey, Orlagh last_name: Creevey - first_name: Rafael A. full_name: García, Rafael A. last_name: García - first_name: Rasmus full_name: Handberg, Rasmus last_name: Handberg - first_name: Daniel full_name: Huber, Daniel last_name: Huber - first_name: Steven D. full_name: Kawaler, Steven D. last_name: Kawaler - first_name: Mikkel N. full_name: Lund, Mikkel N. last_name: Lund - first_name: Travis S. full_name: Metcalfe, Travis S. last_name: Metcalfe - first_name: Keivan G. full_name: Stassun, Keivan G. last_name: Stassun - first_name: Michäel full_name: Bazot, Michäel last_name: Bazot - first_name: Paul G. full_name: Beck, Paul G. last_name: Beck - first_name: Keaton J. full_name: Bell, Keaton J. last_name: Bell - first_name: Maria full_name: Bergemann, Maria last_name: Bergemann - first_name: Derek L. full_name: Buzasi, Derek L. last_name: Buzasi - first_name: Othman full_name: Benomar, Othman last_name: Benomar - first_name: Diego full_name: Bossini, Diego last_name: Bossini - first_name: Lisa Annabelle full_name: Bugnet, Lisa Annabelle id: d9edb345-f866-11ec-9b37-d119b5234501 last_name: Bugnet orcid: 0000-0003-0142-4000 - first_name: Tiago L. full_name: Campante, Tiago L. last_name: Campante - first_name: Zeynep Çelik full_name: Orhan, Zeynep Çelik last_name: Orhan - first_name: Enrico full_name: Corsaro, Enrico last_name: Corsaro - first_name: Lucía full_name: González-Cuesta, Lucía last_name: González-Cuesta - first_name: Guy R. full_name: Davies, Guy R. last_name: Davies - first_name: Maria Pia full_name: Di Mauro, Maria Pia last_name: Di Mauro - first_name: Ricky full_name: Egeland, Ricky last_name: Egeland - first_name: Yvonne P. full_name: Elsworth, Yvonne P. last_name: Elsworth - first_name: Patrick full_name: Gaulme, Patrick last_name: Gaulme - first_name: Hamed full_name: Ghasemi, Hamed last_name: Ghasemi - first_name: Zhao full_name: Guo, Zhao last_name: Guo - first_name: Oliver J. full_name: Hall, Oliver J. last_name: Hall - first_name: Amir full_name: Hasanzadeh, Amir last_name: Hasanzadeh - first_name: Saskia full_name: Hekker, Saskia last_name: Hekker - first_name: Rachel full_name: Howe, Rachel last_name: Howe - first_name: Jon M. full_name: Jenkins, Jon M. last_name: Jenkins - first_name: Antonio full_name: Jiménez, Antonio last_name: Jiménez - first_name: René full_name: Kiefer, René last_name: Kiefer - first_name: James S. full_name: Kuszlewicz, James S. last_name: Kuszlewicz - first_name: Thomas full_name: Kallinger, Thomas last_name: Kallinger - first_name: David W. full_name: Latham, David W. last_name: Latham - first_name: Mia S. full_name: Lundkvist, Mia S. last_name: Lundkvist - first_name: Savita full_name: Mathur, Savita last_name: Mathur - first_name: Josefina full_name: Montalbán, Josefina last_name: Montalbán - first_name: Benoit full_name: Mosser, Benoit last_name: Mosser - first_name: Andres Moya full_name: Bedón, Andres Moya last_name: Bedón - first_name: Martin Bo full_name: Nielsen, Martin Bo last_name: Nielsen - first_name: Sibel full_name: Örtel, Sibel last_name: Örtel - first_name: Ben M. full_name: Rendle, Ben M. last_name: Rendle - first_name: George R. full_name: Ricker, George R. last_name: Ricker - first_name: Thaíse S. full_name: Rodrigues, Thaíse S. last_name: Rodrigues - first_name: Ian W. full_name: Roxburgh, Ian W. last_name: Roxburgh - first_name: Hossein full_name: Safari, Hossein last_name: Safari - first_name: Mathew full_name: Schofield, Mathew last_name: Schofield - first_name: Sara full_name: Seager, Sara last_name: Seager - first_name: Barry full_name: Smalley, Barry last_name: Smalley - first_name: Dennis full_name: Stello, Dennis last_name: Stello - first_name: Róbert full_name: Szabó, Róbert last_name: Szabó - first_name: Jamie full_name: Tayar, Jamie last_name: Tayar - first_name: Nathalie full_name: Themeßl, Nathalie last_name: Themeßl - first_name: Alexandra E. L. full_name: Thomas, Alexandra E. L. last_name: Thomas - first_name: Roland K. full_name: Vanderspek, Roland K. last_name: Vanderspek - first_name: Walter E. full_name: van Rossem, Walter E. last_name: van Rossem - first_name: Mathieu full_name: Vrard, Mathieu last_name: Vrard - first_name: Achim full_name: Weiss, Achim last_name: Weiss - first_name: Timothy R. full_name: White, Timothy R. last_name: White - first_name: Joshua N. full_name: Winn, Joshua N. last_name: Winn - first_name: Mutlu full_name: Yıldız, Mutlu last_name: Yıldız citation: ama: Chaplin WJ, Serenelli AM, Miglio A, et al. Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi. Nature Astronomy. 2020;4(4):382-389. doi:10.1038/s41550-019-0975-9 apa: Chaplin, W. J., Serenelli, A. M., Miglio, A., Morel, T., Mackereth, J. T., Vincenzo, F., … Yıldız, M. (2020). Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi. Nature Astronomy. Springer Nature. https://doi.org/10.1038/s41550-019-0975-9 chicago: Chaplin, William J., Aldo M. Serenelli, Andrea Miglio, Thierry Morel, J. Ted Mackereth, Fiorenzo Vincenzo, Hans Kjeldsen, et al. “Age Dating of an Early Milky Way Merger via Asteroseismology of the Naked-Eye Star ν Indi.” Nature Astronomy. Springer Nature, 2020. https://doi.org/10.1038/s41550-019-0975-9. ieee: W. J. Chaplin et al., “Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi,” Nature Astronomy, vol. 4, no. 4. Springer Nature, pp. 382–389, 2020. ista: Chaplin WJ, Serenelli AM, Miglio A, Morel T, Mackereth JT, Vincenzo F, Kjeldsen H, Basu S, Ball WH, Stokholm A, Verma K, Mosumgaard JR, Silva Aguirre V, Mazumdar A, Ranadive P, Antia HM, Lebreton Y, Ong J, Appourchaux T, Bedding TR, Christensen-Dalsgaard J, Creevey O, García RA, Handberg R, Huber D, Kawaler SD, Lund MN, Metcalfe TS, Stassun KG, Bazot M, Beck PG, Bell KJ, Bergemann M, Buzasi DL, Benomar O, Bossini D, Bugnet LA, Campante TL, Orhan ZÇ, Corsaro E, González-Cuesta L, Davies GR, Di Mauro MP, Egeland R, Elsworth YP, Gaulme P, Ghasemi H, Guo Z, Hall OJ, Hasanzadeh A, Hekker S, Howe R, Jenkins JM, Jiménez A, Kiefer R, Kuszlewicz JS, Kallinger T, Latham DW, Lundkvist MS, Mathur S, Montalbán J, Mosser B, Bedón AM, Nielsen MB, Örtel S, Rendle BM, Ricker GR, Rodrigues TS, Roxburgh IW, Safari H, Schofield M, Seager S, Smalley B, Stello D, Szabó R, Tayar J, Themeßl N, Thomas AEL, Vanderspek RK, van Rossem WE, Vrard M, Weiss A, White TR, Winn JN, Yıldız M. 2020. Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi. Nature Astronomy. 4(4), 382–389. mla: Chaplin, William J., et al. “Age Dating of an Early Milky Way Merger via Asteroseismology of the Naked-Eye Star ν Indi.” Nature Astronomy, vol. 4, no. 4, Springer Nature, 2020, pp. 382–89, doi:10.1038/s41550-019-0975-9. short: W.J. Chaplin, A.M. Serenelli, A. Miglio, T. Morel, J.T. Mackereth, F. Vincenzo, H. Kjeldsen, S. Basu, W.H. Ball, A. Stokholm, K. Verma, J.R. Mosumgaard, V. Silva Aguirre, A. Mazumdar, P. Ranadive, H.M. Antia, Y. Lebreton, J. Ong, T. Appourchaux, T.R. Bedding, J. Christensen-Dalsgaard, O. Creevey, R.A. García, R. Handberg, D. Huber, S.D. Kawaler, M.N. Lund, T.S. Metcalfe, K.G. Stassun, M. Bazot, P.G. Beck, K.J. Bell, M. Bergemann, D.L. Buzasi, O. Benomar, D. Bossini, L.A. Bugnet, T.L. Campante, Z.Ç. Orhan, E. Corsaro, L. González-Cuesta, G.R. Davies, M.P. Di Mauro, R. Egeland, Y.P. Elsworth, P. Gaulme, H. Ghasemi, Z. Guo, O.J. Hall, A. Hasanzadeh, S. Hekker, R. Howe, J.M. Jenkins, A. Jiménez, R. Kiefer, J.S. Kuszlewicz, T. Kallinger, D.W. Latham, M.S. Lundkvist, S. Mathur, J. Montalbán, B. Mosser, A.M. Bedón, M.B. Nielsen, S. Örtel, B.M. Rendle, G.R. Ricker, T.S. Rodrigues, I.W. Roxburgh, H. Safari, M. Schofield, S. Seager, B. Smalley, D. Stello, R. Szabó, J. Tayar, N. Themeßl, A.E.L. Thomas, R.K. Vanderspek, W.E. van Rossem, M. Vrard, A. Weiss, T.R. White, J.N. Winn, M. Yıldız, Nature Astronomy 4 (2020) 382–389. date_created: 2022-07-18T13:36:19Z date_published: 2020-04-01T00:00:00Z date_updated: 2022-08-22T07:08:29Z day: '01' doi: 10.1038/s41550-019-0975-9 extern: '1' external_id: arxiv: - '2001.04653' intvolume: ' 4' issue: '4' keyword: - Astronomy and Astrophysics language: - iso: eng main_file_link: - open_access: '1' url: https://arxiv.org/abs/2001.04653 month: '04' oa: 1 oa_version: Preprint page: 382-389 publication: Nature Astronomy publication_identifier: eissn: - 2397-3366 publication_status: published publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 4 year: '2020' ...