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Relationships between the X-ray and radio behavior of black hole X-ray binaries during outbursts have established a fundamental coupling between the accretion disks and radio jets in these systems. I begin by reviewing the prevailing paradigm for this disk-jet coupling, also highlighting what we know about similarities and differences with neutron star and white dwarf binaries. Until recently, this paradigm had not been directly tested with dedicated high-angular resolution radio imaging over entire outbursts. Moreover, such high-resolution monitoring campaigns had not previously targetted outbursts in which the compact object was either a neutron star or a white dwarf. To address this issue, we have embarked on the Jet Acceleration and Collimation Probe Of Transient X-Ray Binaries (JACPOT XRB) project, which aims to use high angular resolution observations to compare disk-jet coupling across the stellar mass scale, with the goal of probing the importance of the depth of the gravitational potential well, the stellar surface and the stellar magnetic field, on jet formation. Our team has recently concluded its first monitoring series, including (E)VLA, VLBA, X-ray, optical, and near-infrared observations of entire outbursts of the black hole candidate H 1743-322, the neutron star system Aquila X-1, and the white dwarf system SS Cyg. Here I present preliminary results from this work, largely confirming the current paradigm, but highlighting some intriguing new behavior, and suggesting a possible difference in the jet formation process between neutron star and black hole systems.
Growth hormone (GH) is essential for body growth but as normal growth occurs over a relatively short time period and GH secretion continues throughout life it is not surprising that GH has many other functions including both acute and chronic effects on protein metabolism and body composition. Many of the actions of GH are mediated both directly and indirectly through insulin-like growth-factor-I (IGF-I) acting in an endocrine or paracrine manner.
The balance between the rates of protein synthesis and breakdown determines whether the body is in protein balance, protein loss or protein gain (Figure 8.1). The change in these rates in response to physiological and pathological processes is determined by non-hormonal factors, for example, nutritional status, exercise, growth and infection, and hormonal factors. During growth in young animals, protein synthetic rates and protein breakdown rates are higher than in adult animals and the increased protein breakdown may allow the remodelling of muscle enabling growth to take place (1). During muscle hypertrophy induced by exercise both protein synthesis and breakdown increase but synthesis exceeds breakdown and there is a net gain of lean body mass (LBM) (2). Conversely during starvation both rates of protein synthesis and breakdown decrease but breakdown exceeds synthesis and there is a net loss of LBM (3). In acute serious illness the resultant catabolic state is due predominantly to an increased rate of protein degradation (4).
It is customary to refer to body composition as consisting of the fat mass (fat) and the LBM (consisting of predominantly protein). LBM does not change when protein synthesis and breakdown are in balance.
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