نتایج جستجو برای: پوشش wc 12co

تعداد نتایج: 31139  

2000
H. Olofsson

We present observations of circumstellar millimetrewave 13CO line emission towards a sample of 20 cool carbon stars. Using a detailed radiative transfer model we estimate the circumstellar 12CO/13CO-ratios, which we believe accurately measure the important stellar 12C/13C-ratios. For those optically bright carbon stars where it is possible, our derived 12C/13Cratios are compared with the photos...

پایان نامه :وزارت علوم، تحقیقات و فناوری - دانشگاه صنعتی اصفهان 1388

هاردمتال های wc-co به دلیل دارا بودن دو خاصیت سختی و انعطاف پذیری بالا به صورت توأمان، از جایگاه ویژه ای در صنعت برخوردار هستند. اما مقاومت خوردگیِ کم محدودیت هایی برای کاربرد این مواد ایجاد می کند. کامپوزیت های جدید wc-feal-b از نظر رفتار سایشی و مکانیکی خواص بهتری نسبت به هاردمتال های تجاری wc با پایه ی کبالت از خود نشان داده اند و از این رو به عنوان کاندیدی مناسب برای جایگزینی هاردمتال های تج...

2009
R. Visser

Aims. Photodissociation by UV light is an important destruction mechanism for carbon monoxide (CO) in many astrophysical environments, ranging from interstellar clouds to protoplanetary disks. The aim of this work is to gain a better understanding of the depth dependence and isotope-selective nature of this process. Methods. We present a photodissociation model based on recent spectroscopic dat...

2016
Hongxian Xie Xiaoyan Song Fuxing Yin Yongguang Zhang

The effect of coherency WC/Co phase boundaries on the fracture toughness of the nanocrystalline WC-Co cemented carbides is studied by MD simulation method. The simulation results show that the nanocrystalline WC-Co cemented carbides with coherency WC/Co phase boundaries has higher fracture toughness than that without coherency WC/Co phase boundaries. Moreover, the mechanism of why coherency WC/...

2002
A. C. A. Boogert M. R. Hogerheijde G. A. Blake

We explore the infrared M-band (4.7 lm) spectrum of the Class I protostar L1489 IRS in the Taurus molecular cloud. This is the highest-resolution wide-coverage spectrum at this wavelength of a low-mass protostar observed to date (R = 25,000; Dv = 12 km s 1). A large number of narrow absorption lines of gasphase 12CO, 13CO, and C18O are detected, as well as a prominent band of solid 12CO. The ga...

Journal: :Obesity facts 2012
Mohamed Ali Saafi Delphine Frere-Meunier Léonard Feasson Nadia Boutahar Christian Denis

AIM To compare the maximal power output (MPO) of subjects presenting a central adiposity to those of controls and to study the links between plasma leptin or indices of insulin sensitivity (QUICKI) and physical fitness (PF). METHODS MPO was determined for 169 middle-aged men divided into two groups according to waist circumference (WC- < 94 cm, WC+ ≥ 94 cm) each subdivided in two subgroups wi...

2013
Márcio Weissheimer Lauria Lívia Maria Pinheiro Moreira George Luiz Lins Machado-Coelho Raimundo Marques do Nascimento Neto Maria Marta Sarquis Soares Adauto Versiani Ramos

BACKGROUND Body mass index (BMI) and waist circumference (WC) are the most used anthropometric measures to identify obesity. While BMI is considered to be a simple and accurate estimate of general adiposity, WC is an alternative surrogate measure of visceral obesity. However, WC is subject to significant inter-examiner variation. The aim of the present study was to correlate BMI and WC measures...

Journal: :Publications of the Astronomical Society of Japan 2022

We conducted observations and analyses of the molecular cloud, N4, which is located at ~40 pc from SS433 same line sight as that radio shell, in 12CO(J=1-0), 12CO(J=3-2), 13CO(J=3-2), grand-state OH emissions.N4 has a strong gradient integrated intensity 12CO(J=1-0, 3-2) emission northern, eastern western edges. The main body N4 also velocity ~0.16 km s^-1 20"^-1. A shift by up to 3 systemic ~4...

2008
T. Kamiński M. Miller R. Tylenda

Aims. We investigate the structure of a field around the position of V838 Mon as seen in the lowest CO rotational transitions. We also measure and analyse emission in the same lines at the position of V838 Mon. Methods. Observations have primarily been done in the 12CO J = 2→1 and J = 3→2 lines using the KOSMA telescope. A field of 3.4 squared degrees has been mapped in the on-the-fly mode in t...

نمودار تعداد نتایج جستجو در هر سال

با کلیک روی نمودار نتایج را به سال انتشار فیلتر کنید