Search Results - "binary star"

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    Follow Up of GW170817 and Its Electromagnetic Counterpart by Australian-Led Observing Programmes by Anderson, Gemma, Bland, Philip, Booler, Tom, Crosse, Brian, Cupák, Martin, de Gois, J.S., Devillepoix, Hadrien, Emrich, David, Franzen, Thomas, Hancock, Paul, Hartig, Ben, Horsley, L., Howie, Robert, Kenney, David, Paxman, Jonathan, Sansom, Eleanor, Shannon, Ryan, Sokolowski, Marcin, Steele, K., Tingay, Steven, Towner, Martin, Trott, Cathryn, Walker, Mia, Wayth, Randall, Williams, Andrew

    Published 2017
    “…The displacement (~2.2 kpc) of the binary star system from the centre of the main galaxy is not unusual for stars in the host galaxy or stars originating in the merging galaxy, and therefore any constraints on the kick velocity imparted to the progenitor are poor.…”
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  9. 9

    Follow up of GW170817 and its electromagnetic counterpart by Australian-led observing programmes by Andreoni, I., Ackley, K., Cooke, J., Acharyya, A., Allison, J.R., Anderson, G.E., Ashley, M.C.B., Baade, D., Bailes, M., Bannister, K., Beardsley, A., Bessell, M.S., Bian, F., Bland, P.A., Boer, M., Booler, T., Brandeker, A., Brown, I.S., Buckley, D.A.H., Chang, S.-W., Coward, D.M., Crawford, S., Crisp, H., Crosse, B., Cucchiara, A., Cupák, M., de Gois, J.S., Deller, A., Devillepoix, H.A.R., Dobie, D., Elmer, E., Emrich, D., Farah, W., Farrell, T.J., Franzen, T., Gaensler, B.M., Galloway, D.K., Gendre, B., Giblin, T., Goobar, A., Green, J., Hancock, P.J., Hartig, B.A.D., Howell, E.J., Horsley, L., Hotan, A., Howie, R.M., Hu, L., Hu, Y., James, C.W., Johnston, S., Johnston-Hollitt, M., Kaplan, D.L., Kasliwal, M., Keane, E.F., Kenney, D., Klotz, A., Lau, R., Laugier, R., Lenc, E., Li, X., Liang, E., Lidman, C., Luvaul, L.C., Lynch, C., Ma, B., Macpherson, D., Mao, J., McClelland, D.E., McCully, C., Möller, A., Morales, M.F., Morris, D., Murphy, T., Noysena, K., Onken, C.A., Orange, N.B., Osłowski, S., Pallot, D., Paxman, J., Potter, S.B., Pritchard, T., Raja, W., Ridden-Harper, R., Romero-Colmenero, E., Sadler, E.M., Sansom, E.K., Scalzo, R.A., Schmidt, B.P., Scott, S.M., Seghouani, N., Shang, Z., Shannon, R.M., Shao, L., Shara, M.M., Sharp, R., Sokolowski, M., Sollerman, J., Staff, J., Steele, K., Sun, T., Suntzeff, N.B., Tao, C., Tingay, S., Towner, M.C., Thierry, P., Trott, C., Tucker, B.E., Väisänen, P., Krishnan, V. Venkatraman, Walker, M., Wang, L., Wang, X., Wayth, R., Whiting, M., Williams, A., Williams, T., Wolf, C., Wu, C., Wu, X., Yang, J., Yuan, X., Zhang, H., Zhou, J., Zovaro, H.

    Published 2017
    “…The displacement (~2.2 kpc) of the binary star system from the centre of the main galaxy is not unusual for stars in the host galaxy or stars originating in the merging galaxy, and therefore any constraints on the kick velocity imparted to the progenitor are poor.…”
    Get full text
  10. 10

    Constraints on primordial black hole dark matter from wide binaries in the galactic halo by Tyler, Emily Sarah

    Published 2022
    “…These constraints could also be made more reliable by using a larger catalog of binary stars, such as a subset of GAIA DR2.…”
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    Two stellar-mass black holes in the globular cluster M22 by Strader, J., Chomiuk, L., Maccarone, T., Miller-Jones, James, Seth, A.

    Published 2012
    “…Some observational support for this idea is provided by the lack of X-ray-emitting binary stars comprising one black hole and one other star (‘black-hole/X-ray binaries’) in Milky Way globular clusters, even though many neutron-star/X-ray binaries are known. …”
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