Zobrazeno 1 - 10
of 93
pro vyhledávání: '"Toalá, Jesús A."'
Autor:
Tejeda, Emilio, Toalá, Jesús A.
The Bondi-Hoyle-Lyttleton (BHL) accretion model is widely used to describe how a compact object accretes material from a companion's stellar wind in binary systems. However, this classical model becomes inaccurate when the wind velocity ($v_\mathrm{w
Externí odkaz:
http://arxiv.org/abs/2411.01755
Autor:
Van de Steene, Griet, van Hoof, Peter, Kimeswenger, Stefan, Hajduk, Marcin, Tafoya, Daniel, Toala, Jesus, Zijlstra, Albert, Barria, Daniela
Optical spectra of the Very Late Thermal Pulse (VLTP) object V4334 Sgr have shown a rapidly changing spectrum resulting from shocks in the outflow, which created a new bipolar nebula inside the old nebula. We see C II and C III emission lines emergin
Externí odkaz:
http://arxiv.org/abs/2409.13289
Autor:
Hajduk, Marcin, van Hoof, Peter A. M., Zijlstra, Albert A., Van de Steene, Griet, Kimeswenger, Stefan, Barría, Daniela, Tafoya, Daniel, Toalá, Jesús A.
Publikováno v:
A&A 688, L21 (2024)
The very late thermal pulse (VLTP) affects the evolution of $\sim$20\% of 1--8\,$\mathrm M_\odot$ stars, repeating the last phases of the red giant within a few years and leading to the formation of a new, but hydrogen-poor nebula within the old plan
Externí odkaz:
http://arxiv.org/abs/2407.18020
AGB stars are not expected to be X-ray-emitters, yet a small fraction of them, the so-called X-AGBs, show X-ray emission that can be attributed to coronal activity of a companion or accretion onto it. By searching the recently released eROSITA-DE eRA
Externí odkaz:
http://arxiv.org/abs/2407.10552
Spectroscopic observations have shown for decades that the Wolf-Rayet (WR) phenomenon is ubiquitous among stars with different initial masses. Although much effort to understand the winds from massive WR stars has been presented in the literature, no
Externí odkaz:
http://arxiv.org/abs/2405.10177
We present the analysis of publicly available NuSTAR, Suzaku and XMM-Newton observations of the symbiotic recurrent nova T CrB covering the 2006.77-2022.66 yr period. The X-ray spectra are analysed by adopting a model that includes a reflection compo
Externí odkaz:
http://arxiv.org/abs/2405.08980
Autor:
Toalá, Jesús A.
X-ray-emitting symbiotic stars exhibit a variety of spectral shapes classified as $\alpha$, $\beta$, $\gamma$, $\delta$ and $\beta$/$\delta$ types, which have been attributed to different phenomena such as thermonuclear burning on the surface of the
Externí odkaz:
http://arxiv.org/abs/2401.02318
Autor:
Corrales, Lia, Stassun, Keivan G., Cunningham, Tim, Duvvuri, Girish, Drake, Jeremy J., Espaillat, Catherine, Feinstein, Adina D., Gallo, Elena, Gunther, Hans Moritz, King, George W., Kounkel, Marina, Lisse, Carey M., Montez Jr., Rodolfo, Principe, David A., Toala, Jesus A., Wolk, Scott J., Cilley, Raven, Daylan, Tansu, Karovska, Margarita, Pradhan, Pragati, Wheatley, Peter J., Yang, Jun
One of the key research themes identified by the Astro2020 decadal survey is Worlds and Suns in Context. The Advanced X-ray Imaging Satellite (AXIS) is a proposed NASA APEX mission that will become the prime high-energy instrument for studying star-p
Externí odkaz:
http://arxiv.org/abs/2311.07674
The superbubbles (SBs) carved in the interstellar medium by stellar winds and supernovae (SNe) are filled with hot ($T>$10$^{6}$~K) gas that produces soft X-ray emission (0.3-2.0\,keV). Models that assume a constant density medium and central SNe eve
Externí odkaz:
http://arxiv.org/abs/2310.01531
Autor:
Tafoya, Daniel, van Hoof, Peter A. M., Toala, Jesus A., Van de Steene, Griet, Randall, Suzanna, Unnikrishnan, Ramlal, Kimeswenger, Stefan, Hajduk, Marcin, Barria, Daniela, Zijlstra, Albert
We present high angular-resolution observations of Sakurai's object using the Atacama Large Millimeter Array, shedding new light on its morpho-kinematical structure. The millimetre continuum emission, observed at an angular resolution of 20 milliarcs
Externí odkaz:
http://arxiv.org/abs/2308.08962