Astronomical Distance Determination in the Space Age: Secondary Distance Indicators

The formal division of the distance indicators into primary and secondary leads to difficulties in description of methods which can actually be used in two ways: with, and without the support of the other methods for scaling. Thus instead of concentrating on the scaling requirement we concentrate on all methods of distance determination to extragalactic sources which are designated, at least formally, to use for individual sources. Among those, the Supernovae Ia is clearly the leader due to its enormous success in determination of the expansion rate of the Universe. However, new methods are rapidly developing, and there is also a progress in more traditional methods. We give a general overview of the methods but we mostly concentrate on the most recent developments in each field, and future expectations. © 2018, The Author(s)

Microtubule Asymmetry during Neutrophil Polarization and Migration

The development of cell polarity in response to chemoattractant stimulation in human polymorphonuclear neutrophils (PMNs) is characterized by the rapid conversion from round to polarized morphology with a leading lamellipod at the front and a uropod at the rear. During PMN polarization, the microtubule (MT) array undergoes a dramatic reorientation toward the uropod that is maintained during motility and does not require large-scale MT disassembly or cell adhesion to the substratum. MTs are excluded from the leading lamella during polarization and motility, but treatment with a myosin light chain kinase inhibitor (ML-7) or the actin-disrupting drug cytochalasin D causes an expansion of the MT array and penetration of MTs into the lamellipod. Depolymerization of the MT array before stimulation caused 10% of the cells to lose their polarity by extending two opposing lateral lamellipodia. These multipolar cells showed altered localization of a leading lamella-specific marker, talin, and a uropod-specific marker, CD44. In summary, these results indicate that F-actin– and myosin II-dependent forces lead to the development and maintenance of MT asymmetry that may act to reinforce cell polarity during PMN migration