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UW Canis Majoris - Wikipedia
UW Canis Majoris A is a rare blue supergiant of spectral type O7.5-8 Iab. The precise characteristics of the system are still uncertain, in part because the spectral signature of the secondary is very hard to disentangle from the …
About: UW Canis Majoris - DBpedia Association
UW Canis Majoris is a star in the constellation Canis Major. It is classified as a Beta Lyrae eclipsing contact binary and given the variable star designation UW Canis Majoris. Its …
Canis Major - Wikipedia
Canis Major is a prominent constellation because of its many bright stars. These include Sirius (Alpha Canis Majoris), the brightest star in the night sky, as well as three other stars above magnitude 2.0. Furthermore, two other stars are thought to have previously outshone all others in the night sky—Adhara (Epsilon Canis Majoris) shone at −3.99 around 4.7 million years ago, and Mirzam (Beta Cani…
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UW Canis Majoris - Wikiwand
UW Canis Majoris A is a rare blue supergiant of spectral type O7.5-8 Iab. The precise characteristics of the system are still uncertain, in part because the spectral signature of the …
Canis Major: Stars, Myth, Facts, Location, Deep Sky Objects ...
See more on constellation-guide.comCanis Major is the 43rd biggest constellation in the sky, occupying an area of 380 square degrees. It is located in the second quadrant of the southern celestial hemisphere (SQ1). The entire constellation can be seen from locations between the latitudes +60° and -90°. The neighboring constellations are Columba, Lepus, Mo…Mass flow and evolution of UW Canis Majoris - NASA Technical …
The mass flow seems to be basically in the form of a stellar wind emanating from the O7f primary component, with radiation pressure as the controlling factor. The main characteristics that …
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The ultraviolet spectrum of UW Canis Majoris - NASA Technical …
High resolution spectra of the eclipsing binary UW CMa have been obtained in the wavelength range 950 to 3200 A with the Copernicus (OAO-3) and IUE satellites. UW CMa is an …
UW Canis Majoris - alcyone.de
These are binary systems with orbital planes so close to the observer's line of sight (the inclination i of the orbital plane to the plane orthogonal to the line of sight is close to 90 deg) that the …
UW Canis Majoris - Wikidata
The spectrum of the eclipsing binary 29 UW Canis Majoris. O7. E,SB. 4 references. stated in. A two-dimensionnal quantitative spectral classification of 283 O5-B7 stars and the construction …
29 Canis Majoris displays a feature common to a number of early type binaries, namely, a variation in the line intensities in the sense that the lines are weaker when the stellar velocities …
VY Canis Majoris - Wikipedia
VY Canis Majoris (abbreviated to VY CMa) is an extreme oxygen-rich red hypergiant or red supergiant (O-rich RHG or RSG) and pulsating variable star 1.2 kiloparsecs (3,900 light-years) from the Solar System in the slightly southern …
29 UW CANIS MAJORIS* O. Struve, J. Sahade, V. Zebergs, and B. T. Lynds Berkeley Astronomical Department University of California The orbit of this close spectroscopic binary …
UW Canis Majoris – Constellation Guide
Feb 20, 2023 · The Tau Canis Majoris Cluster is a bright open cluster located 4,830 light-years away in the constellation Canis Major. With an apparent magnitude of 3.8,… Read More »
Mass loss from UW Canis Majoris - NASA Technical Reports …
Copernicus satellite measurements of resonance features in the FUV spectrum of the O 7 supergiant UW Canis Majoris (= HD 57060) are compared with theoretical P Cygni profiles. …
Canis Major - Galaxy Map
Sharpless 310 is ionised by two multiple star systems (Tau Canis Majoris and UW Canis Majoris) each made up of several O-class stars. According to a 1997 paper there are at least 5 visually …
Tau Canis Majoris Cluster (NGC 2362) – Constellation Guide
Feb 20, 2023 · UW Canis Majoris is the second brightest star appearing in the same line of sight as the Tau CMa Cluster. It is a close binary system catalogued as a Beta Lyrae variable. The …
UW Canis Majoris - Alchetron, The Free Social Encyclopedia
Dec 13, 2024 · UW Canis Majoris is a star in the constellation Canis Major. It is classified as a Beta Lyrae eclipsing contact binary and given the variable star designation UW Canis Majoris. …
UW Canis Majoris – Wikipedia
UW Canis Majoris eller HD 57060, är en dubbelstjärna i mellersta delen av stjärnbilden Stora hunden. Den har en minsta skenbar magnitud av ca 5,33 [3] och är svagt synlig för blotta ögat …
Sh 2-310 - Galaxy Map
This vast nebula, one of the largest single HII regions known in the Milky Way, is ionised by two multiple star systems (Tau Canis Majoris and UW Canis Majoris) each made up of several O …
UW Canis Majoris | The Universe of The Universe Wiki | Fandom
UW Canis Majoris is a Blue Supergiant in the Constellation Canis Major and has an Eclipsing Contact Binary Companion called UW Canis Majoris B. He was one of the first eclipsing …
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