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"This is the first book dedicated to Husserl's aesthetics. Paul Crowther pieces together Husserl's ideas of phantasy and image and presents them as a unified and innovative account of aesthetic consciousness. He also shows how Husserl's ideas can be developed to solve problems in aesthetics, especially those related to visual art, literature, theatre, and nature. After outlining the major components of Husserl's phenomenological method, Crowther addresses the scope and structure of Husserl's notion of aesthetic consciousness. For Husserl, aesthetic consciousness in all its forms involves phantasy-where items or states of affairs are represented as if actually perceived or experienced, even though they are not, in fact, given in the present perceptual field. Husserl also makes some extraordinarily interesting links between aesthetic consciousness and nature, showing how natural things and environments become instigators of such consciousness when apprehended in the appropriate terms. This "unreality" of the object of aesthetic consciousness anticipates contemporary debates about pictorial representation and is also relevant to Husserl's accounts of literature and theatre. The Phenomenology of Aesthetic Consciousness and Phantasy will appeal to scholars and advanced students interested in aesthetics, philosophy of art, phenomenological aesthetics, and Husserl's philosophy"--

In this paper some key dangers presented by patterns of existence in the postmodern lifework are identified. These dangers consist of symbolic arrest, epistemological nihilism, & technological innovations such as cyborgs & "artilects." It is further argued that such dangers can be obviated by a refoundational philosophical response. (A response of this kind is one that links cognition to constants bond up with the nature of human embodiment, but which allows that these constants are activated in contrasting ways under different historical conditions.). 15 References. Adapted from the source document.

The presence of massive stars (MSs) in the region close to the Galactic Centre (GC) poses several questions about their origin. The harsh environment of the GC favours specific formation scenarios, each of which should imprint characteristic kinematic features on the MSs. We present a 2D kinematic analysis of MSs in a GC region surrounding Sgr A* based on high-precision proper motions obtained with the Hubble Space Telescope. Thanks to a careful data reduction, well-measured bright stars in our proper-motion catalogues have errors better than 0.5 mas yr−1. We discuss the absolute motion of the MSs in the field and their motion relative to Sgr A*, the Arches, and the Quintuplet. For the majority of the MSs, we rule out any distance further than 3–4 kpc from Sgr A* using only kinematic arguments. If their membership to the GC is confirmed, most of the isolated MSs are likely not associated with either the Arches or Quintuplet clusters or Sgr A*. Only a few MSs have proper motions, suggesting that they are likely members of the Arches cluster, in agreement with previous spectroscopic results. Line-of-sight radial velocities and distances are required to shed further light on the origin of most of these massive objects. We also present an analysis of other fast-moving objects in the GC region, finding no clear excess of high-velocity escaping stars. We make our astro-photometric catalogues publicly available. ; ML and AB acknowledge support from STScI grants GO 12915 and 13771. DJL acknowledges support from the Spanish Government Ministerio de Ciencia, Innovación y Universidades through grants PGC-2018-091 3741-B-C22 and from the Canarian Agency for Research, Innovation and Information Society (ACIISI), of the Canary Islands Government, and the European Regional Development Fund (ERDF), under grant with reference ProID2017010115. LRP acknowledges support from the Generalitat Valenciana through the grant PROMETEO/2019/041. LRB acknowledges partial support by MIUR under PRIN programme no. 2017Z2HSMF.