Guinness World Records 2017 book included massive overcontact binary VFTS 352 that was found in Tarantula Survey. (Quotation is not correct, but still cool this reached popular press so well. Clearly thanks to Luis Calçadaincredible artist impression.) `
Ylva’ Götberg’s paper has been accepted for publication in the journal Astronomy and Astrophysics. Find a link to the forthcoming paper here. She computed the first tailor made models for the structure, evolution and atmospheres of the very hot stars that can from in binary systems when a star loses its envelope by interaction with a companion. She shows that these stars emit most of their light as ionizing photons, at wavelengths so short that none of the currently existing astronomical facilities can actually detect them. This first paper explores how metallicity affects these stars, i.e. are stripped stars in our own galaxy different from stripped stars that formed in the early days of the universe when there were less metals available? Stay tuned for more. Further papers to come out soon.
All stars lose mass, in part in the form of a stellar wind. (Even our sun does so, which most known for the beautiful aurora that can be seen) How strong these winds are is not known very well. Measurements are affected by uncertainties such as how smooth or how clumped such winds are. Mathieu Renzo undertook a very careful study to investigate how the various prescriptions for stellar winds and their uncertainties affect the final mass and structure of stars. His paper is accepted for publication and can be obtained here.
A team of astronomers led by Raffaella Margutti (Northwestern University) , including Manos Zapartas, PhD student at the University of Amsterdam, have found a most peculiar supernova explosion, SN2014C, one that defies all established categories of how astronomers thought explosions look like. … Read More »
Tijdens deze voordracht laten sterrenkundigen Selma de Mink (UvA) en Samayra Straal (ASTRON/UvA) je kennismaken met de exotische levens van zware sterren. Ze vertellen over het dramatische einde van het leven van dit soort sterren en hoe ze hun leven na de explosie voortzetten. In het bijzonder gaan ze in op hoe ze radiostraling en de pas waargenomen zwaartekrachtsgolven gebruiken om meer te weten te komen over dit soort sterren.
Datum en tijd: woensdag 26 oktober 2016, 20:00 – 21:30
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Extreme Ultraviolet (UV) light is blocked by our atmosphere (fortunately for us, because they are dangerous for our skin). Even from space it is very hard to measure. At the moment there is no single satellite telescope that can give information about this part of the spectrum. Bad news for astronomers, because they really want to know how many of such ionizing photons are emitted by massive stars. Such photons play a very important role in heating their surrounding clouds where low mass stars and their planets are still forming. These photons are also believed to have played a very big role early in the history of our Universe. They ionized the intergalactic H during the Cosmic Epoch of reionization. This made our universe transparent and ended the so-called Cosmic Dark Ages.
For this study we use a trick proposed by Scoville & Murchikova (2013) that allows to indirectly measure the extreme UV using ALMA. ALMA is an array of antennas in the dry desert of Chile (image), which can observe the sky in (sub)millimeter wavelengths, i.e. in wavelengths that are too red to see with the naked eye. Instead of measuring the ionizing photons directly, we will measure the effect they have on the surrounding H and He gas by measuring the “high-order recombination lines” that ALMA is sensitive too.
This proposal ALMA 2016.1.01015.S (PI De Mink) has been awarded 6.6 hours. The project design and analysis is lead by E. Muchicova (Caltech) under supervision of N. Scoville (Caltech). Image credit: Credit ALMA/NAOJ/NRAO J. Hills
New results from a large extensive survey of the TMBM (Tarantula Massive Binary Monitoring) survey (PI H. Sana) contain data for over a hundred massive hot binary stars, the largest homogeneous sample to date and the first of this size outside our own galaxy. In the first paper, Leonardo Almeida, presents the survey and first results. The They show that the properties are very similar as found in earlier studies. These results point at binarity being a universal phenomenon for massive stars.
The paper “The Tarantula Massive Binary Monitoring: I. Observational campaign and OB-type spectroscopic binaries” by L.A. Almeida, H. Sana, W. Taylor, R. Barbá, A. Bonanos, P. Crowther, A. Damineli, A. de Koter, S.E. de Mink, C.J. Evans, M. Gieles, N.J. Grin, V. Hénault-Brunet, N. Langer, D. Lennon, S. Lockwood, J. Maíz Apellániz, A.F.J. Moffat, C. Neijssel, C. Norman, O.H. Ramírez-Agudelo, N.D. Richardson, A. Schootemeijer, T. Shenar, I. Soszyński, F. Tramper & J.S. Vink is available on the arxiv.
Natalie Wolchover’s, writer at Quanta Magazine, covered the discussion going on among astrophysicist debating the origin of the Binary Black Holes found by LIGO. Find a link to her article and podcast here.
Colliding Black Holes Tell New Story of Stars
Theory predicts that rotating massive stars “get stirred”, bringing elements from the deep center to the surface. Nathan Grin, former MSc student in Amsterdam, now PhD student in Bonn tried to test the model predictions. He analyzed the spectra of more than 72 massive hot giant stars in the Tarantula nebula to determine their surface composition. In particular he looked at the nitrogen abundance, which is known to be a good tracer of mixing processes.
Many of the slowly rotating stars in the sample show surprisingly high levels of nitrogen, much higher than the theory predict. This is worrying, since this group comprises about a third of the sample. Nathan also tried to measure nitrogen for the rapidly rotating stars, but with the current data only upper limits could be determined. Additional spectra will be needed for the full picture.
His paper “The VLT-FLAMES Tarantula Survey XXV. Surface nitrogen abundances of O-type giants and supergiants” has been accepted for publication in Astronomy & Astrophysics. The team consists of N.J. Grin, O.H. Ramirez-Agudelo, A. de Koter, H. Sana, J. Puls, I. Brott, P.A. Crowther, P.L. Dufton, C.J. Evans, G. Graefener, A. Herrero, N. Langer, D.J. Lennon, J.Th. van Loon, N. Markova, S.E. de Mink, F. Najarro, F.R.N. Schneider, W.D. Taylor, F. Tramper, J.S. Vink, W.R. Walborn