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Profil bibliographique

Y. L. Tuo

Informations fournies par OpenAlex. Research Africa ne déduit ni nationalité, ni poste, ni coordonnées personnelles.

5Publications signalées
4Citations signalées
1Affiliations récentes

Les institutions déclarées

Les domaines associés

Astrophysical Phenomena and ObservationsPulsars and Gravitational Waves ResearchGamma-ray bursts and supernovaeAstronomical Observations and InstrumentationAstrophysics and Cosmic Phenomena

Les publications récentes

Accès ouvert 2025 article OpenAlex

Observation on the therapeutic effect of a modified Devine procedure with subcutaneous sliding fixation method for concealed penis

Mohanad Al-Qaisi, Haifu Tian, Jia-Jin Feng, Keming Chen et autres

ABSTRACT: To evaluate the therapeutic effect of a modified Devine procedure with a subcutaneous sliding fixation method for the treatment of congenital concealed penis, we retrospectively selected 45 patients with congenital concealed penises who were admitted to General Hospital of Ningxia Medical …

cn (code pays fourni par la source)

0 citations Asian Journal of Andrology
Accès ouvert 2022 preprint OpenAlex

Monte-Carlo simulations on possible collimation effects of outflows to fan-beamed emission of ultraluminous accreting X-ray pulsars

X. Hou, Yanru You, L. Ji, R. Soria et autres

Pulsating ultraluminous X-ray sources (PULXs) are accreting pulsars with apparent X-ray luminosity exceeding $10^{39}\, \rm erg\ s^{-1}$. We perform Monte-Carlo simulations to investigate whether high collimation effect (or strong beaming effect) is dominant in the presence of accretion outflows, for the fan …

0 citations arXiv (Cornell University)
Accès ouvert 2022 preprint OpenAlex

Fan beamed X-ray emission from 1 keV to above 130 keV from the ultraluminous X-ray pulsar RX J0209.6-7427 in the Small Magellanic Cloud

X. Hou, M. Y. Ge, L. Ji, S. N. Zhang et autres

We present detailed timing and spectral analyses of the transient X-ray pulsar RX J0209.6$-$7427 in the Small Magellanic Cloud during its 2019 giant outburst. With a better known distance than most galactic X-ray pulsars, its peak luminosity is determined to be $(1.11\pm0.06)\times …

1 citation arXiv (Cornell University)
Accès ouvert 2020 preprint OpenAlex

Insight-HXMT insight into switch of the accretion mode: the case of the X-ray pulsar 4U 1901+03

Y. L. Tuo, Long Ji, Sergey S. Tsygankov, T. Mihara et autres

We use the In data collected during the 2019 outburst from X-ray pulsar 4U 1901+03 to complement the orbital parameters reported by Fermi/GBM. Using the Insight-HXMT, we examine the correlation between the derivative of the intrinsic spin frequency and bolometric flux based …

3 citations arXiv (Cornell University)

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