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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 …

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 …

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 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 …

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. …

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 …

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 »

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 …

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 …

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 …

Jan 8, 2007 · Astronomers have studied VY Canis Majoris for more than a century. The star is located 5,000 light-years away. It is 500,000 times brighter and about 30 to 40 times more …

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 …

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. …

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 …

NGC 2362 is a small compact young open cluster in Canis Major that surrounds bright star Tau Canis Majoris (τ CMa - mag. +4.37). This attractive grouping of 60 stars is packed into an area …