552 research outputs found
A sharper view of the outer Galaxy at 1420 and 408 MHz from the Canadian Galactic Plane Survey II: The catalogue of extended radio sources
A new catalogue of extended radio sources has been prepared based on
arcminute-resolution 1420 MHz images from the Canadian Galactic Plane Survey
(CGPS). The new catalogue provides both 1420 MHz and 408 MHz flux density
measurements on sources found near the Galactic plane in the second quadrant of
our Galaxy. In addition cross-identifications are made with other major radio
catalogues and information is provided to facilitate the recovery of CGPS image
data associated with each catalogued source. Numerous new radio sources are
identified and the catalogue provides a comprehensive summary of both newly
discovered and previously known HII regions and supernova remnants in the outer
Galaxy. The catalogue should be of use both for synoptic studies of Galactic
structure and for placing higher resolution observations, at radio and other
wavelengths, in context.Comment: accepted for publication in MNRAS, 8 pages, 6 figure
A sharper view of the outer Galaxy at 1420 and 408 MHz from the Canadian Galactic Plane Survey - I. Revisiting the KR catalogue and new Gigahertz Peaked Spectrum Sources
Arcminute-resolution radio continuum images at 408 and 1420 MHz from the
Canadian Galactic Plane Survey (CGPS) have been used to reexamine radio sources
listed in the Kallas and Reich (1980) catalogue. This catalogue is of
particular interest to Galactic studies as it lists both extended and compact
radio sources found in the second Galactic quadrant. We have determined the
nature (extended vs. compact, Galactic vs. extragalactic) of all of these
bright radio sources. A number of large HII regions with no optical
counterparts are highlighted along with a sample of large radio galaxies. Many
sources previously thought to be extended Galactic objects are shown to be
point sources. A sample of point sources with flat or rising spectra between
408 and 1420 MHz has been compiled, and within this sample likely Gigahertz
Peaked Spectrum sources have been identified.Comment: 10 pages, 9 figure
Permissible devotion: discovering transitions in the materiality and embodiment of women's faith expressions during the English reformation
This thesis examines five devotional works written for or by women published between 1574 and
1624, spanning the decades that could be described as the transitional period of the religious status quo in
England from Catholicism to Protestantism.
The language of devotion is examined in the light of embodied spirituality, and how this may have
transitioned to a more scriptural and moral piety towards the end of the period. Areas are identified in which
women adjusted their domestic and personal devotional practice so they could retain their religious agency,
as well as perpetuate, in some form, deeply valued devotional practices that had been part of community life
for centuries. It shows that, during the period of the Reformation, the materiality of domestic religious practice
transferred from apotropaic or devotional objects to textual objects that reflected the new emphasis on
scripture and pious morality. In addition, examination of the language used in devotional works identifies
conceptual shifts in women’s understanding of the bodily expressions of their spirituality.Thesis (M.A.
IRAS03063+5735: A Bowshock Nebula Powered by an Early B Star
Mid-infrared images from the Spitzer Space Telescope Galactic Legacy Infrared
MidPlane Survey Extraordinaire program reveal that the infrared source IRAS
03063+5735 is a bowshock nebula produced by an early B star, 2MASS
03101044+5747035. We present new optical spectra of this star, classify it as a
B1.5 V, and determine a probable association with a molecular cloud complex at
V_LSR=-38 -- -42 km/s in the outer Galaxy near l=140.59 degr, b=-0.250 degr. On
the basis of spectroscopic parallax, we estimate a distance of 4.0 +/-1 kpc to
both the bowshock nebula and the molecular complex. One plausible scenario is
that this a high-velocity runaway star impinging upon a molecular cloud. We
identify the HII region and stellar cluster associated with IRAS 03064+5638 at
a projected distance of 64 pc as one plausible birth site. The
spectrophotometric distance and linkage to a molecular feature provides another
piece of data helping to secure the ill-determined rotation curve in the outer
Galaxy. As a by-product of spectral typing this star, we present empirical
spectral diagnostic diagrams suitable for approximate spectral classification
of O and B stars using He lines in the little-used yellow-red portion of the
optical spectrum.Comment: Accepted for publication in the Astronomical Journa
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