Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Sun Y"'
Autor:
Thygesen, E., Sun, Y., Huang, J., Dage, K. C., Zepf, S. E., Kundu, A., Haggard, D., Maccarone, T. J.
Ultraluminous X-ray Sources (ULXs) in globular clusters are low mass X-ray binaries that achieve high X-ray luminosities through a currently uncertain accretion mechanism. Using archival Chandra and Hubble Space Telescope observations, we perform a v
Externí odkaz:
http://arxiv.org/abs/2211.07699
Autor:
Wevers, T., Coughlin, E. R., Pasham, D. R., Guolo, M., Sun, Y., Wen, S., Jonker, P. G., Zabludoff, A., Malyali, A., Arcodia, R., Liu, Z., Merloni, A., Rau, A., Grotova, I., Short, P., Cao, Z.
Stars that interact with supermassive black holes (SMBHs) can either be completely or partially destroyed by tides. In a partial tidal disruption event (TDE) the high-density core of the star remains intact, and the low-density, outer envelope of the
Externí odkaz:
http://arxiv.org/abs/2209.07538
X-ray loud M dwarfs are a major source of by-product (contamination) in the X-ray band of the multiwavelength quasar survey (MWQS). As a by-product, the low dispersion spectra of 22 M dwarfs are obtained in which the spectra of 16 sources are taken f
Externí odkaz:
http://arxiv.org/abs/1201.1359