Zobrazeno 1 - 10
of 915
pro vyhledávání: '"Degenaar N"'
XMMSL1 J171900.4-353217 is a very-faint X-ray transient that was discovered in 2010 March when it exhibited an outburst. We report on 7 observations, obtained with the X-Ray Telescope (XRT) aboard the Neil Gehrels {\it{Swift}} Observatory between 201
Externí odkaz:
http://arxiv.org/abs/2409.19649
Autor:
Anitra, A., Miceli, C., Di Salvo, T., Iaria, R., Degenaar, N., Miller, M. Jon, Barra, F., Leone, W., Burderi, L.
We propose a novel approach for determining the orbital inclination of low-mass X-ray binary systems by modelling the H$\alpha$ and H$\beta$ line profiles emitted by the accretion disc, with a Newtonian version of diskline. We applied the model to tw
Externí odkaz:
http://arxiv.org/abs/2409.11988
Autor:
Eijnden, J. van den, Robins, D., Sharma, R., Sánchez-Fernández, C., Russell, T. D., Degenaar, N., Miller-Jones, J. C. A., Maccarone, T.
The Rapid Burster is a unique neutron star low-mass X-ray binary system, showing both thermonuclear Type-I and accretion-driven Type-II X-ray bursts. Recent studies have demonstrated how coordinated observations of X-ray and radio variability can con
Externí odkaz:
http://arxiv.org/abs/2405.19827
Autor:
Eijnden, J. van den, Escorial, A. Rouco, Alfonso-Garzón, J., Miller-Jones, J. C. A., Kretschmar, P., Fürst, F., Degenaar, N., Santisteban, J. V. Hernández, Sivakoff, G. R., Russell, T. D., Wijnands, R.
LS V +44 17 is a persistent Be/X-ray binary (BeXRB) that displayed a bright, double-peaked period of X-ray activity in late 2022/early 2023. We present a radio monitoring campaign of this outburst using the Very Large Array. Radio emission was detect
Externí odkaz:
http://arxiv.org/abs/2311.00631
Autor:
Segura, N. Castro, Knigge, C., Matthews, J. H., Vincentelli, F. M., Charles, P., Long, K. S., Altamirano, D., Buckley, D. A. H., Modiano, D., Torres, M. A. P., Buisson, D. J. K., Fijma, S., Alabarta, K., Degenaar, N., Georganti, M., Baglio, M. C.
The evolution of accreting X-ray binary systems is closely coupled to the properties of their donor stars. As a result, we can constrain the evolutionary track a system is by establishing the nature of its donor. Here, we present far-UV spectroscopy
Externí odkaz:
http://arxiv.org/abs/2310.03397
Autor:
Vincentelli, F. M., Casella, P., Borghese, A., Cavecchi, Y., Mastroserio, G., Stella, L., Altamirano, D., Padilla, M. Armas, Baglio, M. C., Belloni, T. M., Casares, J., Cúneo, V. A., Degenaar, N., Trigo, M. Díaz, Fender, R., Maccarone, T., Malzac, J., Sánchez, D. Mata, Middleton, M., Migliari, S., Muñoz-Darias, T., O'Brien, K., Panizo-Espinar, G., Sánchez-Sierras, J., Russell, D. M., Uttley, P.
We report on the first simultaneous high-time resolution X-ray and infrared (IR) observations of a neutron star low mass X-ray binary in its hard state. We performed $\approx 2\,$h of simultaneous observations of 4U 1728-34 using HAWK-I@VLT, XMM-Newt
Externí odkaz:
http://arxiv.org/abs/2308.15570
Autor:
Janssens, S., Shenar, T., Degenaar, N., Bodensteiner, J., Sana, H., Audenaert, J., Frost, A. J.
Publikováno v:
A&A 677, L9 (2023)
Context. MWC 656 was reported as the first known Be star with a black-hole (BH) companion in a 60 d period. The mass of the proposed BH companion is estimated to be between 4 - 7 MSun. This estimate is based on radial velocity (RV) measurements deriv
Externí odkaz:
http://arxiv.org/abs/2308.08642
Autor:
Eijnden, J. van den, Sidoli, L., Trigo, M. Diaz, Degenaar, N., Mellah, I. El, Fürst, F., Grinberg, V., Kretschmar, P., Martínez-Núñez, S., Miller-Jones, J. C. A., Postnov, K., Russell, T. D.
Neutron stars accreting from OB supergiants are often divided between persistently and transiently accreting systems, called Supergiant X-ray Binaries (SgXBs) and Supergiant Fast X-ray Transients (SFXTs). This dichotomy in accretion behaviour is typi
Externí odkaz:
http://arxiv.org/abs/2308.06021
Autor:
Marino, A., Russell, T. D., Del Santo, M., Beri, A., Sanna, A., Zelati, F. Coti, Degenaar, N., Altamirano, D., Ambrosi, E., Anitra, A., Carotenuto, F., D'Ai, A., Di Salvo, T., Manca, A., Motta, S. E., Pinto, C., Pintore, F., Rea, N., Eijnden, J. Van den
The accretion flow / jet correlation in neutron star (NS) low-mass X-ray binaries (LMXBs) is far less understood when compared to black hole (BH) LMXBs. In this paper we will present the results of a dense multi-wavelength observational campaign on t
Externí odkaz:
http://arxiv.org/abs/2307.16566
Autor:
Fijma, S., Segura, N. Castro, Degenaar, N., Knigge, C., Higginbottom, N., Santisteban, J. V. Hernández, Maccarone, T. J.
Accreting low mass X-ray binaries (LMXBs) are capable of launching powerful outflows such as accretion disc winds. In disc winds, vast amounts of material can be carried away, potentially greatly impacting the binary and its environment. Previous stu
Externí odkaz:
http://arxiv.org/abs/2305.10793