Search results
Results: 60
Number of items: 60
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Pauli, D., Oskinova, L. M., Hamann, W.-R., Bowman, D. M., Todt, H., Shenar, T., Sander, A. A. C., Erba, C., Gómez-González, V. M. A., Kehrig, C., Klencki, J., Kuiper, R., Mehner, A., de Mink, S. E., Oey, M. S., Ramachandran, V., Schootemeijer, A., Reyero Serantes, S., & Wofford, A. (2023). Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity. Astronomy and Astrophysics, 673, Article A40. https://doi.org/10.1051/0004-6361/202345881 -
Romagnolo, A., Belczynski, K., Klencki, J., Agrawal, P., Shenar, T., & Szécsi, D. (2023). The role of stellar expansion on the formation of gravitational wave sources. Monthly Notices of the Royal Astronomical Society, 525(1), 706-720. https://doi.org/10.1093/mnras/stad2366 -
Brands, S. A., De Koter, A., Bestenlehner, J. M., Crowther, P. A., Sundqvist, J. O., Puls, J., Caballero-Nieves, S. M., Abdul-Masih, M., Driessen, F. A., García, M., Geen, S., Gräfener, G., Hawcroft, C., Kaper, L., Keszthelyi, Z., Langer, N., Sana, H., Schneider, F. R. N., Shenar, T., & Vink, J. S. (2022). The R136 star cluster dissected with Hubble Space Telescope/STIS. III. The most massive stars and their clumped winds [Data set]. Zenodo. https://doi.org/10.5281/zenodo.6353513
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Shenar, T., Sana, H., Mahy, L., Maíz Apellániz, J., Crowther, P. A., Gromadzki, M., Herrero, A., Langer, N., Marchant, P., Schneider, F. R. N., Sen, K., Soszyński, I., & Toonen, S. (2022). The Tarantula Massive Binary Monitoring VI: Characterisation of hidden companions in 51 single-lined O-type binaries: A flat mass-ratio distribution and black-hole binary candidates. Astronomy and Astrophysics, 665, Article A148. https://doi.org/10.1051/0004-6361/202244245 -
Dsilva, K., Shenar, T., Sana, H., & Marchant, P. (2022). A spectroscopic multiplicity survey of Galactic Wolf-Rayet stars II: The northern WNE sequence. Astronomy and Astrophysics, 664, Article A93. https://doi.org/10.1051/0004-6361/202142729 -
Gayley, K. G., Vink, J. S., ud-Doula, A., David-Uraz, A., Ignace, R., Prinja, R., St-Louis, N., Ekström, S., Nazé, Y., Shenar, T., Scowen, P. A., Sudnik, N., Owocki, S. P., Sundqvist, J. O., Driessen, F. A., & Hennicker, L. (2022). Understanding structure in line-driven stellar winds using ultraviolet spectropolarimetry in the time domain. Astrophysics and Space Science, 367(12), Article 123. https://doi.org/10.1007/s10509-022-04142-6
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Peters, G. J., Gayley, K. G., Ignace, R., Jones, C. E., Nazé, Y., St-Louis, N., Stevance, H., Vink, J. S., Richardson, N. D., Hoffman, J. L., Lomax, J. R., Shenar, T., Fullard, A. G., & Scowen, P. A. (2022). Ultraviolet spectropolarimetry: conservative and nonconservative mass transfer in OB interacting binaries. Astrophysics and Space Science, 367(12), Article 119. https://doi.org/10.1007/s10509-022-04106-w
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Brands, S. A., de Koter, A., Bestenlehner, J. M., Crowther, P. A., Sundqvist, J. O., Puls, J., Caballero-Nieves, S. M., Abdul-Masih, M., Driessen, F. A., García, M. G., Geen, S., Gräfener, G., Hawcroft, C., Kaper, L., Keszthelyi, Z., Langer, N., Sana, H., Schneider, F. R. N., Shenar, T., & Vink, J. S. (2022). The R136 star cluster dissected with Hubble Space Telescope/STIS. III: The most massive stars and their clumped winds. Astronomy & Astrophysics, 663, Article A36. https://doi.org/10.1051/0004-6361/202142742
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Hennicker, L., Kee, N. D., Shenar, T., Bodensteiner, J., Abdul-Masih, M., El Mellah, I., Sana, H., & Sundqvist, J. O. (2022). Binary-object spectral-synthesis in 3D (BOSS-3D): Modelling Hα emission in the enigmatic multiple system LB-1. Astronomy & Astrophysics, 660, Article A17. https://doi.org/10.1051/0004-6361/202141831
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Mahy, L., Sana, H., Shenar, T., Sen, K., Langer, N., Marchant, P., Abdul-Masih, M., Banyard, G., Bodensteiner, J., Bowman, D. M., Dsilva, K., Fabry, M., Hawcroft, C., Janssens, S., Van Reeth, T., & Eldridge, C. (2022). Identifying quiescent compact objects in massive Galactic single-lined spectroscopic binaries. Astronomy and Astrophysics, 664, Article A159. https://doi.org/10.1051/0004-6361/202243147
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