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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 …

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 …

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 …

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 …

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 »

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 …

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 …

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 …

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 …

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. …

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. …

The far-UV spectrum of the eclipsing binary UW CMa (O7f + O-B) had earlier been utilized to derive a mass-loss rate of about 10−6 to 10−5 solar mass per year. The mass flow seems to …

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 …

Positioned 24 arc minutes north of NGC 2362 is UW Canis Majoris (29 CMa), a Beta Lyrae type eclipsing binary star. Magnitude +6.5 open cluster, NGC 2354, is located 1.25 degrees …

The ultraviolet spectrum of the close binary UW CMa, obtained with the Copernicus (OAO-3) and IUE satellites in the wavelength region from 1010 to 1510 A and from 1200 to 3000 A, …

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 …

Canis Major Constellation lies in The Southern Celestial Hemisphere of our night sky. The Brightest Star in our Sky, Sirius, is located in Canis Major. The three known galaxies within …