Zobrazeno 1 - 10
of 3 020
pro vyhledávání: '"You Hua"'
Publikováno v:
Chinese Journal of Contemporary Neurology and Neurosurgery, Vol 21, Iss 04, Pp 281-288 (2021)
Objective To report a case of peroxisomal acyl⁃CoA oxidase (ACOX1) deficiency, which was caused by an unreported mutation of ACOX1 gene, and review its clinical characteristics. Methods and Results The male child patient suffered from neonatal hypo
Externí odkaz:
https://doaj.org/article/a5f798020a3f4471be135a5ddeb06f81
Publikováno v:
Frontiers of Nursing, Vol 7, Iss 4, Pp 321-327 (2021)
To investigate the prevalence of cancer-related depression and anxiety in western China among patients with ovarian cancer and analyze their influencing factors.
Externí odkaz:
https://doaj.org/article/f2418398da9b4f48b47b126d808f359e
Autor:
Points, Sean D., Long, Knox S., Blair, William P., Williams, Rosa, Chu, You-Hua, Winkler, P. Frank, White, Richard L., Rest, Armin, Li, Chuan-Jui, Valdes, Francisco
We have used the Dark Energy Camera (DECam) on the CTIO Blanco 4-m telescope to perform a new emission-line survey of the Large Magellanic Cloud (LMC) using narrow-band H-alpha and [SII] filters in addition to a continuum band for use in creating pur
Externí odkaz:
http://arxiv.org/abs/2409.04846
Supergiant shells (SGSs) are the largest interstellar structures where heated and enriched gas flows into the host galaxy's halo. The SGSs in the Large Magellanic Cloud (LMC) are so close that their stars can be resolved with ground-based telescopes
Externí odkaz:
http://arxiv.org/abs/2405.04024
Autor:
Oey, M. S., Sawant, Amit N., Danehkar, Ashkbiz, Silich, Sergiy, Smith, Linda J., Melinder, Jens, Leitherer, Claus, Hayes, Matthew, Jaskot, Anne E., Calzetti, Daniela, Chu, You-Hua, James, Bethan L., Oestlin, Goeran
Publikováno v:
Astrophys.J.Lett.958:L10,2023
We use the Hubble Space Telescope ACS camera to obtain the first spatially resolved, nebular imaging in the light of C IV 1548,1551 by using the F150LP and F165LP filters. These observations of the local starburst Mrk 71 in NGC 2366 show emission app
Externí odkaz:
http://arxiv.org/abs/2310.13751
Autor:
Smith, Linda J., Oey, M. S., Hernandez, Svea, Ryon, Jenna, Leitherer, Claus, Charlot, Stephane, Bruzual, Gustavo, Calzetti, Daniela, Chu, You-Hua, Hayes, Matthew J., James, Bethan L., Jaskot, Anne. E., Oestlin, Goeran
Mrk 71 is a low metallicity (Z = 0.16 Z_sun) starburst region in the local dwarf galaxy NGC 2366, hosting two super star clusters (SSCs A and B), and is recognized as a Green Pea (GP) analog with SSC A responsible for the GP properties. We present ST
Externí odkaz:
http://arxiv.org/abs/2310.03413
Autor:
Chen, Wei-An, Li, Chuan-Jui, Chu, You-Hua, Ueda, Shutaro, Wang, Kuo-Song, Liu, Sheng-Yuan, Chen, Bo-An
The supernova remnant (SNR) 30 Dor B is associated with the \ion{H}{2} region ionized by the OB association LH99. The complex interstellar environment has made it difficult to study the physical structure of this SNR. We have used Hubble Space Telesc
Externí odkaz:
http://arxiv.org/abs/2309.13313
Autor:
Kim, Hyosun, Lee, Ho-Gyu, Ohyama, Youichi, Kim, Ji Hoon, Scicluna, Peter, Chu, You-Hua, Mauron, Nicolas, Ueta, Toshiya
Publikováno v:
Proceedings of the International Astronomical Union, 17(S370), 78-83 (2023)
Recent abrupt changes of CW Leonis may indicate that we are witnessing the moment that the central carbon star is evolving off the Asymptotic Giant Branch (AGB) and entering into the pre-planetary nebula (PPN) phase. The recent appearance of a red co
Externí odkaz:
http://arxiv.org/abs/2308.15679
Despite the 30-year history of ultra-luminous X-ray sources (ULXs) studies, issues like the majority of their physical natures (i.e., neutron stars, stellar-mass black holes, or intermediate black holes) as well as the accretion mechanisms are still
Externí odkaz:
http://arxiv.org/abs/2308.06287
Autor:
De Marco, Orsola, Akashi, Muhammad, Akras, Stavros, Alcolea, Javier, Aleman, Isabel, Amram, Philippe, Balick, Bruce, De Beck, Elvire, Blackman, Eric G., Boffin, Henri M. J., Boumis, Panos, Bublitz, Jesse, Bucciarelli, Beatrice, Bujarrabal, Valentin, Cami, Jan, Chornay, Nicholas, Chu, You-Hua, Corradi, Romano L. M., Frank, Adam, Garcia-Segura, Guillermo, Garcia-Hernandez, D. A., Garcia-Rojas, Jorge, Gomez-Llanos, Veronica, Goncalves, Denise R., Guerrero, Martin A., Jones, David, Karakas, Amanda I., Kastner, Joel H., Kwok, Sun, Lykou, Foteini, Manchado, Arturo, Matsuura, Mikako, McDonald, Iain, Monreal-Ibero, Ana, Monteiro, Hektor, Baez, Paula Moraga, Morisset, Christophe, Miszalski, Brent, Mohamed, Shazrene S., Montez Jr., Rodolfo, Nordhaus, Jason, de Oliveira, Claudia Mendes, Osborn, Zara, Otsuka, Masaaki, Parker, Quentin A., Peeters, Els, Quint, Bruno C., Quintana-Lacaci, Guillermo, Redman, Matt, Ruiter, Ashley J., Sabin, Laurence, Contreras, Carmen Sanchez, Santander-Garcia, Miguel, Seitenzahl, Ivo, Sahai, Raghvendra, Soker, Noam, Speck, Angela K., Stanghellini, Letizia, Steffen, Wolfgang, Toala, Jesus A., Ueta, Toshiya, Van de Steene, Griet, Villaver, Eva, Ventura, Paolo, Vlemmings, Wouter, Walsh, Jeremy R., Wesson, Roger, van Winckel, Hans, Zijlstra, Albert A.
Publikováno v:
Nature Astronomy, 2022, Vol. 6, p. 1421
Planetary nebulae (PNe), the ejected envelopes of red giant stars, provide us with a history of the last, mass-losing phases of 90 percent of stars initially more massive than the Sun. Here, we analyse James Webb Space Telescope (JWST) Early Release
Externí odkaz:
http://arxiv.org/abs/2301.02775