S.E. de Mink
Identifiers
- name variant S.E. de Mink 0.60 · backfill
Papers (48)
- Stellar properties of observed stars stripped in binaries in the Magellanic Clouds astro-ph.SR · 2023 · author #9
- X-Shooting ULLYSES: massive stars at low metallicity. I. Project Description astro-ph.SR · 2023 · author #65
- Nucleosynthesis of binary-stripped stars astro-ph.SR · 2023 · author #4
- The VLT-FLAMES Tarantula Survey: Observational evidence for two distinct populations of massive runaway stars in 30 Doradus astro-ph.SR · 2022 · author #12
- JWST Imaging of Earendel, the Extremely Magnified Star at Redshift $z=6.2$ astro-ph.GA · 2022 · author #4
- The cosmic carbon footprint of massive stars stripped in binary systems astro-ph.SR · 2021 · author #3
- The contribution from stars stripped in binaries to cosmic reionization of hydrogen and helium astro-ph.GA · 2019 · author #2
- The impact of stars stripped in binaries on the integrated spectra of stellar populations astro-ph.GA · 2019 · author #2
- Response to comment on "An excess of massive stars in the local 30 Doradus starburst" astro-ph.SR · 2018 · author #15
- The VLT-FLAMES Tarantula Survey. XXIX. Massive star formation in the local 30 Doradus starburst astro-ph.SR · 2018 · author #14
- Gaia DR2 reveals a very massive runaway star ejected from R136 astro-ph.SR · 2018 · author #7
- An excess of massive stars in the local 30 Doradus starburst astro-ph.SR · 2018 · author #15
- Legacy ExtraGalactic UV Survey with The Hubble Space Telescope. Stellar cluster catalogues and first insights into cluster formation and evolution in NGC 628 astro-ph.GA · 2017 · author #31
- Delay-time distribution of core-collapse supernovae with late events resulting from binary interaction astro-ph.HE · 2017 · author #2
- The Tarantula Massive Binary Monitoring: I. Observational campaign and OB-type spectroscopic binaries astro-ph.SR · 2016 · author #9
- The VLT-FLAMES Tarantula Survey XXV. Surface nitrogen abundances of O-type giants and supergiants astro-ph.SR · 2016 · author #16
- The R136 star cluster dissected with Hubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of HeII 1640 in young star clusters astro-ph.SR · 2016 · author #11
- Hubble Tarantula Treasury Project. III. Photometric Catalog and Resulting Constraints on the Progression of Star Formation in the 30 Doradus Region astro-ph.GA · 2015 · author #19
- Discovery of the massive overcontact binary VFTS 352: Evidence for enhanced internal mixing astro-ph.SR · 2015 · author #3
- The VLT-FLAMES Tarantula Survey XXI. Stellar spin rates of O-type spectroscopic binaries astro-ph.SR · 2015 · author #3
- Massive stars on the verge of exploding: the properties of oxygen sequence Wolf-Rayet stars astro-ph.SR · 2015 · author #9
- On the formation and evolution of the first Be star in a black hole binary MWC 656 astro-ph.HE · 2015 · author #4
- Evolution of Mass Functions of Coeval Stars through Wind Mass Loss and Binary Interactions astro-ph.SR · 2015 · author #4
- The evolution of rotating very massive stars with LMC composition astro-ph.SR · 2015 · author #4
- Rotational velocities of single and binary O-type stars in the Tarantula Nebula astro-ph.SR · 2014 · author #5
- The incidence of stellar mergers and mass gainers among massive stars astro-ph.SR · 2013 · author #1
- On the nature of the WO3 star DR1 in IC 1613 astro-ph.SR · 2013 · author #11
- On the nature of WO stars: a quantitative analysis of the WO3 star DR1 in IC 1613 astro-ph.SR · 2013 · author #11
- Rotational properties of the O-type star population in the Tarantula region astro-ph.SR · 2013 · author #6
- Early Disc Accretion as the Origin of Abundance Anomalies in Globular Clusters astro-ph.GA · 2013 · author #3
- The VLT-FLAMES Tarantula Survey XII. Rotational velocities of the single O-type stars astro-ph.SR · 2013 · author #6
- The elusive origin of Carbon-Enhanced Metal-Poor stars astro-ph.SR · 2013 · author #5
- Wind Roche-lobe overflow: Application to carbon-enhanced metal-poor stars astro-ph.SR · 2013 · author #5
- The VLT-FLAMES Tarantula Survey X: Evidence for a bimodal distribution of rotational velocities for the single early B-type stars astro-ph.SR · 2012 · author #6
- Multiplicity of massive O stars and evolutionary implications astro-ph.SR · 2012 · author #2
- Discovery of a magnetic field in the rapidly-rotating O-type secondary of the colliding-wind binary HD 47129 (Plaskett's star) astro-ph.SR · 2012 · author #12
- The VLT-FLAMES Tarantula Survey: The fastest rotating O-type star and shortest period LMC pulsar - remnants of a supernova disrupted binary? astro-ph.SR · 2011 · author #7
- Binary progenitor models of type IIb supernovae astro-ph.SR · 2011 · author #2
- Binaries are the best single stars astro-ph.SR · 2010 · author #1
- Light elements in massive single and binary stars astro-ph.SR · 2010 · author #4
- Massive binaries and the enrichment of the interstellar medium in globular clusters astro-ph.SR · 2009 · author #1
- A new evolutionary scenario for the formation of massive black-hole binaries such as M33 X-7 and IC 10 X-1 astro-ph.SR · 2009 · author #1
- Massive binaries as the source of abundance anomalies in globular clusters astro-ph.SR · 2009 · author #1
- Rotational mixing in massive binaries: detached short-period systems astro-ph.SR · 2009 · author #1
- Rotational mixing in close binaries astro-ph · 2008 · author #1
- Rotation and massive close binary evolution astro-ph · 2008 · author #7
- Binaries at Low Metallicity: ranges for case A, B and C mass transfer astro-ph · 2007 · author #1
- Efficiency of mass transfer in massive close binaries, Tests from double-lined eclipsing binaries in the SMC astro-ph · 2007 · author #1
Mentions
- 2305.06376 #65 · arxiv_oai · confidence 0.70 S.E. de Mink
- 2307.00074 #9 · arxiv_oai · confidence 0.70 S.E. de Mink
- 2303.04520 #4 · arxiv_oai · confidence 0.70 S.E. de Mink
- 2211.13476 #12 · arxiv_oai · confidence 0.70 S.E. de Mink
- 2208.09007 #4 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1807.09816 #15 · arxiv_oai · confidence 0.70 S.E. de Mink
- 2110.04131 #3 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1911.00543 #2 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1908.06102 #2 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1805.08277 #7 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1807.03821 #14 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1801.03107 #15 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1705.01588 #31 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1701.07032 #2 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1609.00197 #16 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1610.03500 #9 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1603.04994 #11 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1511.06021 #19 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1509.08940 #3 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1507.00839 #9 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1507.02286 #3 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1504.03146 #4 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1409.1822 #5 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1312.3650 #1 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1310.2849 #11 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1309.3566 #3 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1309.2929 #6 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1302.4441 #5 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1212.2424 #6 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1209.6326 #12 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1111.0157 #7 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1102.1732 #2 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1504.01735 #4 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1003.1575 #4 · arxiv_oai · confidence 0.70 S.E. de Mink
- 0910.3767 #1 · arxiv_oai · confidence 0.70 S.E. de Mink
- 0910.1086 #1 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1501.03794 #4 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1312.1555 #11 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1309.7250 #6 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1304.2570 #5 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1211.4740 #2 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1010.2200 #1 · arxiv_oai · confidence 0.70 S.E. de Mink
- 0902.1751 #1 · arxiv_oai · confidence 0.70 S.E. de Mink
- 0805.2544 #1 · arxiv_oai · confidence 0.70 S.E. de Mink
- 0803.0621 #7 · arxiv_oai · confidence 0.70 S.E. de Mink
- astro-ph/0703480 #1 · arxiv_oai · confidence 0.70 S.E. de Mink
- 0910.3694 #1 · arxiv_oai · confidence 0.70 S.E. de Mink
- 0710.1010 #1 · arxiv_oai · confidence 0.70 S.E. de Mink
- 1511.06021 #19 · backfill · confidence 0.70 S.E. de Mink
- 1509.08940 #3 · backfill · confidence 0.70 S.E. de Mink
- 1507.02286 #3 · backfill · confidence 0.70 S.E. de Mink
- 1507.00839 #9 · backfill · confidence 0.70 S.E. de Mink
- 1504.03146 #4 · backfill · confidence 0.70 S.E. de Mink
- 1504.01735 #4 · backfill · confidence 0.70 S.E. de Mink
- 1501.03794 #4 · backfill · confidence 0.70 S.E. de Mink
- 1409.1822 #5 · backfill · confidence 0.70 S.E. de Mink
- 1312.3650 #1 · backfill · confidence 0.70 S.E. de Mink
- 1312.1555 #11 · backfill · confidence 0.70 S.E. de Mink
- 1310.2849 #11 · backfill · confidence 0.70 S.E. de Mink
- 1309.7250 #6 · backfill · confidence 0.70 S.E. de Mink
- 1309.3566 #3 · backfill · confidence 0.70 S.E. de Mink
- 1309.2929 #6 · backfill · confidence 0.70 S.E. de Mink
- 1304.2570 #5 · backfill · confidence 0.70 S.E. de Mink
- 1302.4441 #5 · backfill · confidence 0.70 S.E. de Mink
- 1212.2424 #6 · backfill · confidence 0.70 S.E. de Mink
- 1211.4740 #2 · backfill · confidence 0.70 S.E. de Mink
- 1209.6326 #12 · backfill · confidence 0.70 S.E. de Mink
- 1111.0157 #7 · backfill · confidence 0.70 S.E. de Mink
- 1102.1732 #2 · backfill · confidence 0.70 S.E. de Mink
- 1010.2200 #1 · backfill · confidence 0.70 S.E. de Mink
- 1003.1575 #4 · backfill · confidence 0.70 S.E. de Mink
- 0910.3767 #1 · backfill · confidence 0.70 S.E. de Mink
- 0910.3694 #1 · backfill · confidence 0.70 S.E. de Mink
- 0910.1086 #1 · backfill · confidence 0.70 S.E. de Mink
- 0902.1751 #1 · backfill · confidence 0.70 S.E. de Mink
- 0805.2544 #1 · backfill · confidence 0.70 S.E. de Mink
- 0803.0621 #7 · backfill · confidence 0.70 S.E. de Mink
- 0710.1010 #1 · backfill · confidence 0.70 S.E. de Mink
Frequent Coauthors
- N. Langer 29 shared papers
- H. Sana 23 shared papers
- A. de Koter 21 shared papers
- C.J. Evans 17 shared papers
- J.S. Vink 17 shared papers
- A. Herrero 14 shared papers
- D.J. Lennon 13 shared papers
- R.G. Izzard 13 shared papers
- F. Tramper 12 shared papers
- G. Gr\"afener 12 shared papers
- F.R.N. Schneider 11 shared papers
- O.H. Ram\'irez-Agudelo 10 shared papers
- O.R. Pols 10 shared papers
- J. Ma\'iz Apell\'aniz 9 shared papers
- P.A. Crowther 9 shared papers
- I. Brott 8 shared papers
- N. Markova 8 shared papers
- S. Sim\'on-D\'iaz 8 shared papers
- F. Najarro 7 shared papers
- J. Puls 7 shared papers