Search Results - "Fogantini, F A"

The variable radio counterpart of Swift J1858.6-0814 by van den Eijnden, J, Degenaar, N, Russell, T D, Buisson, D J K, Altamirano, D, Armas Padilla, M, Bahramian, A, Castro Segura, N, Fogantini, F A, Heinke, C O, Maccarone, T, Maitra, D, Miller-Jones, J C A, Muñoz-Darias, T, Özbey Arabacı, M, Russell, D M, Shaw, A W, Sivakoff, G, Tetarenko, A J, Vincentelli, F, Wijnands, R

“…ABSTRACT Swift J1858.6-0814 is a transient neutron star X-ray binary discovered in 2018 October. Multiwavelength follow-up observations across the…”
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Soft X-ray emission lines in the X-ray binary Swift J1858.6–0814 observed with XMM–Newton Reflection Grating Spectrometer: disc atmosphere or wind? by Buisson, D J K, Altamirano, D, Díaz Trigo, M, Mendez, M, Armas Padilla, M, Castro Segura, N, Degenaar, N D, van den Eijnden, J, Fogantini, F A, Gandhi, P, Knigge, C, Muñoz-Darias, T, Özbey Arabacı, M, Vincentelli, F M

“…ABSTRACT We find soft X-ray emission lines from the X-ray binary Swift J1858.6–0814 in data from XMM–NewtonReflection Grating Spectrometer (RGS): N vii, O vii,…”
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Soft X-ray emission lines in the X-ray binary Swift J1858.6-0814 observed with XMM-Newton-RGS: disc atmosphere or wind? by Buisson, D. J. K, Altamirano, D, Trigo, M. Díaz, Mendez, M, Padilla, M. Armas, Segura, N. Castro, Degenaar, N. D, Eijnden, J. van den, Fogantini, F. A, Gandhi, P, Knigge, C, Muñoz-Darias, T, Arabacı, M. Özbey, Vincentelli, F. M

“…We find soft X-ray emission lines from the X-ray binary Swift J1858.6-0814 in data from XMM-Newton-RGS: N VII, O VII and O VIII, as well as notable residuals…”
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The variable radio counterpart of Swift J1858.6-0814 by Eijnden, J. van den, Degenaar, N, Russell, T. D, Buisson, D. J. K, Altamirano, D, Padilla, M. Armas, Bahramian, A, Segura, N. Castro, Fogantini, F. A, Heinke, C. O, Maccarone, T, Maitra, D, Miller-Jones, J. C. A, Muñoz-Darias, T, Arabacı, M. Özbey, Russell, D. M, Shaw, A. W, Sivakoff, G, Tetarenko, A. J, Vincentelli, F, Wijnands, R

“…Swift J1858.6-0814 is a transient neutron star X-ray binary discovered in October 2018. Multi-wavelength follow-up observations across the electromagnetic…”
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The Changing-look Optical Wind of the Flaring X-ray Transient Swift J1858.6-0814 by Muñoz-Darias, T, Padilla, M. Armas, Jiménez-Ibarra, F, Panizo-Espinar, G, Casares, J, Altamirano, D, Buisson, D. J. K, Segura, N. Castro, Cúneo, V. A, Degenaar, N, Fogantini, F. A, Knigge, C, Sánchez, D. Mata, Arabaci, M. Özbey, Sánchez-Sierras, J, Torres, M. A. P, Eijnden, J. van den, Vincentelli, F. M

“…We present the discovery of an optical accretion disk wind in the X-ray transient Swift J1858.6-0814. Our 90-spectrum data set, taken with the 10.4m GTC…”
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