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G Protein Pathways, Part B: G Proteins and Their Regulators
This volume covers topics such as the structure and identification of functional domains of G proteins, and activation of G proteins by receptors or other regulators. The text takes an integrated approach to studying common experimental questions at many different levels related to G proteins. Methods related to G proteins using molecular modeling, systems biology, protein engineering, protein biochemistry, cell biology, and physiology are all accessible in the same volume. The critically acclaimed laboratory standard for more than forty years, Methods in Enzymology is one of the most highly respected publications in the field of biochemistry. Since 1955, each volume has been eagerly awaited, frequently consulted, and praised by researchers and reviewers alike. Now with more than 300 volumes (all of them still in print), the series contains much material still relevant today truly an essential publication for researchers in all fields of life sciences.
B/G-Steem - User Manual and CD-ROM
This is a combined self-esteem and locus of control scale that has been developed and standardised in British schools on a population of pupils aged six to 13 years. Special attention has been paid to the use of clear and simple language and the scale only requires Yes/No responses. The test can be administered in two formats: " paper and pencil tick sheets (group or individual) " computer presentation, text and voice with automatic scoring (individual only). Included in the handbook and on CD-ROM are primary and secondary test forms for both boys and girls. All the forms are freely copiable. Full marking and procedure instructions are included. This is a useful resource for evaluating changes in children resulting from new programmes and interventions.
Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars
This book introduces the theory of stellar atmospheres. Almost everything we know about stars is by analysis of the radiation coming from their atmospheres. Several aspects of astrophysics require accurate atmospheric parameters and abundances. Spectroscopy is one of the most powerful tools at an astronomer’s disposal, allowing the determination of the fundamental parameters of stars: surface temperature, gravity, chemical composition, magnetic field, rotation and turbulence. These can be supplemented by distance measurements or pulsation parameters providing information about stellar interior and stellar evolution, otherwise unavailable. The volume is based on lectures presented at the Wrocław's Spectroscopic School aimed at training young researchers in performing quantitative spectral analysis of low-, mid-, and high-resolution spectra of B, A, and F-type stars.
