tshenar [at] tau.ac.il
tomer.shenar [at] gmail.com
TOMER SHENAR
Hello, שלום, hallo, hola, ٱلسَّلَامُ عَلَيْكُمْ! ;-)
My name is Tomer Shenar - an assistant professor at the University of Tel Aviv, Israel.
Looking for a MSc/PhD/postdoc in astrophysics? Join our group!
My research focuses on massive stars. Today, we know that the vast majority of massive stars interact with companion stars during their lifetime: My research is dedicated to study this interaction and its implication on stellar evolution.
I collect and use multi-wavelength spectroscopic, photometric, and interferometric data with the world's largest telescopes to infer the observational properties of massive stars and binaries in the Local Group. I develop and utilise state-of-the-art model atmospheres and spectral disentangling algorithms to derive robust constraints on the progenitors of compact objects (Wolf-Rayet stars, OB-type stars, stripped stars), with the goal of advancing our understanding of the evolution of massive stars and binaries and the production of gravitational-wave sources. I am a co-developer of the Potsdam Wolf-Rayet (PoWR) code.
I am a consortium member of 4MOST, MSE. and E-ELT's MOSAIC, and the PI of the Binarity at LOw Metallicity (BLOeM) ESO Large Programme.
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Jan. 2024: assistant professor, University of Tel Aviv, Israel
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2023 - 2024: group leader, Programa de Atracción de Talento, CAB, Madrid, Spain
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2021 - 2023: Marie-Curie fellow, Uni. Amsterdam, NL
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2018 - 2021: postdoc, KU Leuven, Belgium
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2017-2018: postdoc, Uni. Potsdam, Germany
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2013-2017; PhD (summa cum laude), Uni. Potsdam, Germany
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2011-2013; MSc in Physics, Uni. Potsdam, Germany
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2007-2010: BSc in Mathematics & physics, Technion, Israel
Research highlights:
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PI of ESO Large Programme dedicated to the study of binarity at low metallicity (BLOeM)
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First robust detection of a magnetic Wolf-Rayet star; Shenar et al. 2023, Science, 381, 761
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First discovery of an unambiguous dormant black hole outside our Galaxy; Shenar et al. 2022, Nature Astronomy, 6, 1085
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First evidence for flat mass-ratio distribution at subsolar metallicity; Shenar et al. 2022, A&A, 665, 148)
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Discovery of a new type of post-interaction binaries ("black hole impostors"); Shenar et al. 2020, A&A, 639, 6
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Metallicity-dependent luminosity criteria for the Wolf-Rayet phenomenon; Shenar et al. 2020, A&A, 634, 79
TOMER SHENAR
stellar astrophysicist
Assistant professor, Tel Aviv University
An artist's impression of VFTS 243, the first unambiguous dormant stellar-mass black hole detected outside our Galaxy
Shenar et al. 2022, Nature Astronomy
Image credit: ESO/L. Calçada
(taken from an article in "The Guardian")
Research interests (click to find out more)
Past PhD & MSc students, postdocs
PhD: Karan Dsilva
KU Leuven, BE
Karan takes a modern look at the Galactic Wolf-Rayet stars and tries to understand how they evolved.
WC binaries:
Dsilva, Shenar et al. 2020, A&A, 641, 26
WN binaries:
Dsilva, Shenar et al. 2022, A&A, 664, 93
Dsilva, Shenar et al. 2023, A&A, in press
Karan is now a postdoc in the Gaia team at the Université libre de Bruxelles (ULB), Belgium
PhD: Julila Bodensteiner
KU Leuven, BE
Julia searches for post-interaction binaries in clusters.
Julia finds a clear excess of Be stars in evolved clusters. Together with Julia, we also found some very cool Be stars (confused as black holes) hiding not far away from us!
Julia is now an independent ESO fellow at ESO@Garching
MSc + PhD: Soetkin Janssens
KU Leuven, BE
Soetkin analysed a highly complex Wolf-Rayet "binary" in the Large Magellanic Cloud. "Binary", because she found it's a quadruple or quintuple system, hosting one of the most massive contact systems known
Jannsens, Shenar et al. 2020, A&A, 646, 33
Soetkin now continues her PhD under my co-supervision with the goal of hunting for black holes with Gaia -- check out her 1st PhD paper: Janssens, Shenar et al. 2022, A&A, 658, 129
Janssens, Shenar et al. 2023, A&A, in press
MSc: Roel Lefever
KU Leuven, BE
The majority of Wolf-Rayet analyses assume a fixed wind velocity law. Roel performed a quantitative investigation of alternative velocity laws and their impact on the spectral appearance of Wolf-Rayet stars and their inferred stellar parameters, with important implications on the properties of black-hole progenitors.
Levefer, Sander, Shenar et al., MNRAS, 521, 1374
Roel is now a PhD student with Andreas Sander in Heidelberg, Germany
MSc: Sancho Luijten
University of Amstedam, NL
Sancho will be analysing multi-epoch data acquired with the UVES@ESO spectrograph (PI: Shenar), targeting two very unique WR binaries. These binaries were proposed to host not one, but two Wolf-Rayet stars, and hence potentially correspond to a rare evolutionary phase prior to black-hole + black-hole binary formation. His thesis is available here.
Sancho is a PhD candidate in Barak Zackay's group at the Weizmann Institute
MSc: Ardra Ramachandran
University of Amstedam, NL
Ardra was selected through a competitive process to participate in the ASPIRE summerschool at the Uni. Amsterdam. Her goal? Re-deriving the orbital solution a famous "dormant" black hole in our Galaxy, MWC 656.
Guess what? She found that the unseen companion weighs between 0.7-3 Msun, and hence very unlikely to be a black hole.
Ardra is a PhD student at the University of Warwick, UK
MSc: Freek Temming
University of Amsterdam, NL
Postdoc: Marimar Rubio Díez
El Centro de Astrobiología, Spain
Freek will be working on new data acquired with the X-SHOOTER instrument @ VLT to establish the binary properties and physical properties of the WC population.
Freek found that the properties of the LMC WC stars are comparable to the Galactic ones, as shown in his thesis, soon to be submitted as a peer-reviewed paper.
Freek founded the data analysis company Duracode
Marimar is working on STIS+COS data obtained with the Hubble Space Telescope to study the physical parameters and winds of the WC population in the Large Magellanic Cloud.
Stay tuned!
Current MSc & PhD students & postdocs
MSc: Roey Ovadia
Tel Aviv University, Israel
Roey will focus on the multiplicity of massive stars in the Small Magellanic Cloud using FLAMES/VLT data acquired within the BLOeM survey.
Stay tuned!
Tools & codes (click to access)
The PoWR code & grids
Spectral disentangling @github
Fellowships & third-party funding
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Jan. 2024: Start-up package, Tel Aviv University (1M $)
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Oct. 2022: 5-year group leader position (Programa de Atracción de Talento) at the Centro de Astrobiología (CAB), Madrid, Spain
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Jun. 2021: 3-year senior postdoc FWO fellowship , KU Leuven, Belgium
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Feb. 2021: 2-yr Marie Skłodowska-Curie Individual fellowship, University of Amsterdam, Netherlands
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Aug. 2019: 4-yr FWO PhD fellowship (scientific PI and co-supervisor)
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Sep. 2018: ERC-funded position (PI: Prof. Hugues Sana)
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Jan. 2013: Richard-Winter scholarship for excellency
Prizes & awards:
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Jun. 2021: KU Leuven's Research Council Award
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Mar. 2018; Horizon 2020 Seal of excellence
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Oct. 2017: Carl-Ramsauer award, Berlin Physics society
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Jan. 2017: graduated summa cum laude
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Sep. 2016: visit at the MIT, funded by the Chandra visitor program
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Jul 2014: Physics thesis award, Berlin physical society
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Jul. 2013: Award for outstanding achievements of international students, DAAD
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3-year senior FWO fellowship (PI)
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4-yr FWO PhD fellowship (scientific PI and co-supervisor
PUBLIC OUTREACH
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Skype-a-Scientist (www.skypeascientist.com)
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Activities in kindergartens: Introduction to our solar system
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Mentoring of pupils in astronomy-related projects, at the University of Potsdam, Germany
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Physics & Maths tutoring of pupils with socially or economically disadvantaged background (Elele center, Berlin)
Introducing the children to the solar system
The children draw their own impression of the solar system
The kids "pretended" to be planets revolving around the sun - lots of fun!
The kids were inspired by real pictures and simulations of planets, stars, and galaxies
WHY ASTROPHYSICS?
My fascination for the universe has never left me ever since taking part in an astronomical event in the Negev, a desert in the southern region of Israel, at the age of 14. I learned that all these thousands of bright points in the night sky were suns, much like our own, but in different shapes and sizes. That day I realized that my connection with the stars would accompany me for the rest of my life.
Through my work, I hope to advance our understanding of stars, and inspire young, curious pupils and students to investigate the Universe we live in.
PRIVATE
When I'm not doing science, I read, play the guitar & piano, and I love to sing. I play adventure games, dance, or just hang out with my dear ones. More about me over a beer (or two)!