Neutron Star Extreme Matter Observatory: A kilohertz-band gravitational-wave detector in the global network

Autor: Ackley, K., Adya, V. B., Agrawal, P., Altin, P., Ashton, G., Bailes, M., Baltinas, E., Barbuio, A., Beniwal, D., Blair, C., Blair, D., Bolingbroke, G. N., Bossilkov, V., Boublil, S. Shachar, Brown, D. D., Burridge, B. J., Bustillo, J. Calderon, Cameron, J., Cao, H. Tuong, Carlin, J. B., Chang, S., Charlton, P., Chatterjee, C., Chattopadhyay, D., Chen, X., Chi, J., Chow, J., Chu, Q., Ciobanu, A., Clarke, T., Clearwater, P., Cooke, J., Coward, D., Crisp, H., Dattatri, R. J., Deller, A. T., Dobie, D. A., Dunn, L., Easter, P. J., Eichholz, J., Evans, R., Flynn, C., Foran, G., Forsyth, P., Gai, Y., Galaudage, S., Galloway, D. K., Gendre, B., Goncharov, B., Goode, S., Gozzard, D., Grace, B., Graham, A. W., Heger, A., Vivanco, F. Hernandez, Hirai, R., Holland, N. A., Holmes, Z. J., Howard, E., Howell, E., Howitt, G., Hübner, M. T., Hurley, J., Ingram, C., Hamedan, V. Jaberian, Jenner, K., Ju, L., Kapasi, D. P., Kaur, T., Kijbunchoo, N., Kovalam, M., Choudhary, R. Kumar, Lasky, P. D., Lau, M. Y. M., Leung, J., Liu, J., Loh, K., Mailvagan, A., Mandel, I., McCann, J. J., McClelland, D. E., McKenzie, K., McManus, D., McRae, T., Melatos, A., Meyers, P., Middleton, H., Miles, M. T., Millhouse, M., Mong, Y. Lun, Mueller, B., Munch, J., Musiov, J., Muusse, S., Nathan, R. S., Naveh, Y., Neijssel, C., Neil, B., Ng, S. W. S., Oloworaran, V., Ottaway, D. J., Page, M., Pan, J., Pathak, M., Payne, E., Powell, J., Pritchard, J., Puckridge, E., Raidani, A., Rallabhandi, V., Reardon, D., Riley, J. A., Roberts, L., Romero-Shaw, I. M., Roocke, T. J., Rowell, G., Sahu, N., Sarin, N., Sarre, L., Sattari, H., Schiworski, M., Scott, S. M., Sengar, R., Shaddock, D., Shannon, R., SHI, J., Sibley, P., Slagmolen, B. J. J., Slaven-Blair, T., Smith, R. J. E., Spollard, J., Steed, L., Strang, L., Sun, H., Sunderland, A., Suvorova, S., Talbot, C., Thrane, E., Töyrä, D., Trahanas, P., Vajpeyi, A., van Heijningen, J. V., Vargas, A. F., Veitch, P. J., Vigna-Gomez, A., Wade, A., Walker, K., Wang, Z., Ward, R. L., Ward, K., Webb, S., Wen, L., Wette, K., Willcox, R., Winterflood, J., Wolf, C., Wu, B., Yap, M. Jet, You, Z., Yu, H., Zhang, J., Zhao, C., Zhu, X.

Publikováno v: PASA (2020) 37, e047

Gravitational waves from coalescing neutron stars encode information about nuclear matter at extreme densities, inaccessible by laboratory experiments. The late inspiral is influenced by the presence of tides, which depend on the neutron star equatio

Externí odkaz: http://arxiv.org/abs/2007.03128

The Tarantula Massive Binary Monitoring: I. Observational campaign and OB-type spectroscopic binaries

Autor: Almeida, L. A., Sana, H., Taylor, W., Barbá, R., Bonanos, A., Crowther, P., Damineli, A., de Koter, A., de Mink, S. E., Evans, C. J., Gieles, M., Grin, N. J., Hénault-Brunet, V., Langer, N., Lennon, D., Lockwood, S., Apellániz, J. Maíz, Moffat, A. F. J., Neijssel, C., Norman, C., Ramírez-Agudelo, O. H., Richardson, N. D., Schootemeijer, A., Shenar, T., Soszyński, I., Tramper, F., Vink, J. S.

Publikováno v: A&A 598, A84 (2017)

Massive binaries (MBs) play a crucial role in the Universe. Knowing the distributions of their orbital parameters (OPs) is important for a wide range of topics, from stellar feedback to binary evolution channels, from the distribution of supernova ty

Externí odkaz: http://arxiv.org/abs/1610.03500

Tarantula Massive Binary Monitoring

Autor: Almeida, LA, Sana, H, Taylor, W, Barbá, R, Bonanos, AZ, Crowther, P, Damineli, A, de Koter, A, de Mink, SE, Evans, CJ, Gieles, M, Grin, NJ, Hénault-Brunet, V, Langer, N, Lennon, D, Lockwood, S, Maíz Apellániz, J, Moffat, AFJ, Neijssel, C, Norman, C, Ramírez-Agudelo, OH, Richardson, ND, Schootemeijer, A, Shenar, T, Soszynski, I, Tramper, F, Vink, JS

© ESO, 2017. Context. Massive binaries play a crucial role in the Universe. Knowing the distributions of their orbital parameters is important for a wide range of topics from stellar feedback to binary evolution channels and from the distribution of

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______1131::bd2650237775174ba6b429c9647063f7
https://lirias.kuleuven.be/handle/123456789/564517

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Detecting double neutron stars with LISA

Autor: Alejandro Vigna-Gómez, Ilya Mandel, Coenraad J. Neijssel, Mike Y. M. Lau, Alberto Sesana, S. P. Stevenson

Publikováno v: Lau, M Y M, Mandel, I, Vigna-Gomez, A, Neijssel, C J, Stevenson, S & Sesana, A 2020, ' Detecting double neutron stars with LISA ', Monthly Notices of the Royal Astronomical Society, vol. 492, no. 3, pp. 3061-3072 . https://doi.org/10.1093/mnras/staa002

We estimate the properties of the double neutron star (DNS) population that will be observable by the planned space-based interferometer LISA. By following the gravitational radiation driven evolution of DNSs generated from rapid population synthesis

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::db94ba2b570225169b5d656d7d4a501a
https://doi.org/10.1093/mnras/staa002