Results 111 to 120 of about 181,622 (240)
Radial Velocities of Southern B Stars Determined at the Radcliffe Observatory*: (Paper II) [PDF]
M. W. Feast+2 more
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Surviving in the Hot-Neptune Desert: The Discovery of the Ultrahot Neptune TOI-3261b
The recent discoveries of Neptune-sized ultra-short-period planets (USPs) challenge existing planet formation theories. It is unclear whether these residents of the Hot Neptune Desert have similar origins to smaller, rocky USPs, or if this discrete ...
Emma Nabbie+47 more
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Radial Velocities of Southern B Stars Determined at the Radcliffe Observatory*: (Paper I) [PDF]
M. W. Feast+2 more
openalex +1 more source
Four Sub-Earth Planets Orbiting Barnard’s Star from MAROON-X and ESPRESSO
Barnard’s Star is an old, single M dwarf star that comprises the second-closest extrasolar system. It has a long history of claimed planet detections from both radial velocities and astrometry.
Ritvik Basant+11 more
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Wave-Length Standards for Radial-Velocity Determinations from B-type Spectra [PDF]
R. M. Petrie
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Breaking the degeneracy between warps and radial flows in external galaxies [PDF]
Observations of the line-of-sight component of emitter velocities in galaxies are valuable for reconstructing their 2D velocity fields, albeit requiring certain assumptions. A common one is that radial flows can be neglected in the outer regions of galaxies, while their geometry can be deformed by a warp. A specular approach assumes that galactic discs
arxiv
Radial Velocity Observations of Southern Visual Binaries [PDF]
S. A. Archer
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Fourteen stars whose radial velocities vary
Ralph E. Wilson, Roscoe F. Sanford
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An Emission-Line Object of High Radial Velocity [PDF]
G. H. Herbig, N. U. Mayall
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The precise Doppler method for measuring stellar radial velocities (RV) is a fundamental technique in modern astronomy. This method records a star's spectrum and detects periodic Doppler shifts in its spectral features, which indicate the gravitational influences induced by orbiting companions.
openaire +2 more sources