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3篇 您的检索式:作者名="S.Wolf"
    题名 作者 年代 出处 被引量
1Cancer-directed surgery in malignant pleural mesothelioma: extrapleural pneumonectomy and pleurectomy/decortication显示文摘Malignant pleural mesothelioma(MPM)is a primary solid malignancy related to inhalational asbestos exposure.Despite advances in therapy,MPM remains challenging to treat with a post-treatment survival of only 15%at 5-year.In recent years,extra-pleural pneumonectomy has decreased in popularity due to a high morbidity rate and mortality compared to pleurectomy/decortication and other therapeutic alternatives.In this review,we will discuss both procedures,outcomes,ongoing studies,and the roles of surgery in the future treatment of this disease.Brian Housman Andrea S.Wolf 2021Journal of Cancer Metastasis and Treatment2021,7,1:1
2血管紧张素转化酶抑制剂对慢性肾小球肾炎时蛋白尿的影响显示文摘早在1827年R.Bright就发现了肾脏疾病与浮肿和蛋白尿之间的关系。现已证明,肾脏疾病本身以及全身性疾病时均可出现蛋白尿。蛋白尿的程度仅提示肾功能受损的情况,而与其病因无关。 血管紧张素转化酶抑制剂(ACEI)有助于改善蛋白尿,其机制可能与改变了血压、肾小球内压以及肾小球基底膜通透性有关。 我们给慢性肾小球肾炎性高血压者ACEI,以观察其对尿中蛋白、白蛋白和IgG排清量以及肾脏血流动力学和肾素血管紧张素系统的影响。C.M.Erley E.Komini T.Nicaeus N.Braun S.Wolf T.Risler 王琳 1995德国医学1995,12,1:0
3The Relative Orientation between Local Magnetic Field and Galactic Plane in Low Latitude Dark Clouds显示文摘In this work,we study the magnetic field morphology of selected star-forming clouds spread over the galactic latitude(b)range−10°to 10°.The polarimetric observations of clouds CB24,CB27 and CB188 are conducted to study the magnetic field geometry of those clouds using the 104 cm Sampurnanand Telescope(ST)located at ARIES,Manora Peak,Nainital,India.These observations are combined with those of 14 further low latitude clouds available in the literature.Most of these clouds are located within a distance range 140–500 pc except for CB3(∼2500 pc),CB34(∼1500 pc),CB39(∼1500 pc)and CB60(∼1500 pc).Analyzing the polarimetric data of 17 clouds,we find that the alignment between the envelope magnetic field(θ^(env)_(B))and galactic plane(GP)(θGP)of the low-latitude clouds varies with their galactic longitudes(l).We observe a strong correlation between the longitude(l)and the offset(θ_(off)=|θ^(env)_(B)-θ_(GP))which shows that θ^(env)_(B) is parallel to the GP when the clouds are situated in the region 115°250°.To check the consistency of our results,the stellar polarization data available in the Heiles catalog are overlaid on the DSS image of the clouds having mean polarization vector of field stars.The results are almost consistent with the Heiles data.A systematic discussion is presented in the paper.The effect of turbulence in the cloud is also studied which may play an important role in causing the misalignment phenomenon observed between θ^(env)_(B) and θ_(GP).We have used Herschel(Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.)SPIRE 500μm and SCUBA 850μm dust continuum emission maps in our work to understand the density structure of the clouds.Gulafsha B.Choudhury Himadri S.Das B.J.Medhi J.C.Pandey S.Wolf T.K.Dhar A.M.Mazarbhuiya 2022Research in Astronomy and Astrophysics2022,22,7:0
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