Author: Orren C. Mohler
Publisher:
ISBN:
Category : Spectrum, Solar
Languages : en
Pages : 96
Book Description
A Table of Solar Spectrum Wave Lengths, 11984A to 25578A.
Author: Orren C. Mohler
Publisher:
ISBN:
Category : Spectrum, Solar
Languages : en
Pages : 96
Book Description
Publisher:
ISBN:
Category : Spectrum, Solar
Languages : en
Pages : 96
Book Description
Line Parameters and Computed Spectra for Water Vapor Bands at 2.7
Author: David Murray Gates
Publisher:
ISBN:
Category : Absorption spectra
Languages : en
Pages : 144
Book Description
Publisher:
ISBN:
Category : Absorption spectra
Languages : en
Pages : 144
Book Description
Quarterly Review
Author:
Publisher: UM Libraries
ISBN:
Category :
Languages : en
Pages : 416
Book Description
Includes section: "Some Michigan books."
Publisher: UM Libraries
ISBN:
Category :
Languages : en
Pages : 416
Book Description
Includes section: "Some Michigan books."
An Atlas of the Solar Spectrum in the Infrared from 1850 to 9000 Cm−1 (1.1 to 5.4 Microns), Revised
Author: Lloyd Wallace
Publisher:
ISBN:
Category : Infrared spectra
Languages : en
Pages : 296
Book Description
Publisher:
ISBN:
Category : Infrared spectra
Languages : en
Pages : 296
Book Description
The Johns Hopkins University Circular
Author:
Publisher:
ISBN:
Category :
Languages : en
Pages : 222
Book Description
Includes University catalogues, President's report, Financial report, registers, announcement material, etc.
Publisher:
ISBN:
Category :
Languages : en
Pages : 222
Book Description
Includes University catalogues, President's report, Financial report, registers, announcement material, etc.
Brown Dwarf Companions to Young Solar an
Author: Stanimir Metchev
Publisher: Universal-Publishers
ISBN: 158112290X
Category : Science
Languages : en
Pages : 255
Book Description
We present results from an adaptive optics survey conducted with the Palomar and Keck telescopes over 3 years, which measured the frequency of stellar and sub-stellar companions to Sun-like stars. The survey sample contains 266 stars in the 3-10000 million year age range at heliocentric distances between 8 and 200 parsecs and with spectral types between F5-K5. A sub-sample of 101 stars, between 3-500 million years old, were observed in deep exposures with a coronagraph to search for faint sub-stellar companions. A total of 288 candidate companions were discovered around the sample stars, which were re-imaged at subsequent epochs to determine physical association with the candidate host stars by checking for common proper motion. Benefitting from a highly accurate astrometric calibration of the observations, we were able to successfully apply the common proper motion test in the majority of the cases, including stars with proper motions as small as 20 milli-arcseconds/year. The results from the survey include the discovery of three new brown dwarf companions (HD 49197B, HD 203030B, and ScoPMS 214B), 43 new stellar binaries, and a triple system. The physical association of an additional, a priori-suspected, candidate sub-stellar companion to the star HII 1348 is astrometrically confirmed. The newly-discovered and confirmed young brown dwarf companions span a range of spectral types between M5 and T0.5, and will be of prime significance for constraining evolutionary models of young brown dwarfs and extra-solar planets. Based on the 3 new detections of sub-stellar companions in the 101 star sub-sample and following a careful estimate of the survey incompleteness, a Bayesian statistical analysis shows that the frequency of 0.012-0.072 solar-mass brown dwarfs in 30-1600 AU orbits around young solar analogs is 6.8% (-4.9%, +8.3%; 2-sigma limits). While this is a factor of 3 lower than the frequency of stellar companions to G-dwarfs in the same orbital range, it is significantly higher than the frequency of brown dwarfs in 0-3 AU orbits discovered through precision radial velocity surveys. It is also fully consistent with the observed frequency of 0-3 AU extra-solar planets. Thus, the result demonstrates that the radial-velocity "brown dwarf desert" does not extend to wide separations, contrary to previous belief.
Publisher: Universal-Publishers
ISBN: 158112290X
Category : Science
Languages : en
Pages : 255
Book Description
We present results from an adaptive optics survey conducted with the Palomar and Keck telescopes over 3 years, which measured the frequency of stellar and sub-stellar companions to Sun-like stars. The survey sample contains 266 stars in the 3-10000 million year age range at heliocentric distances between 8 and 200 parsecs and with spectral types between F5-K5. A sub-sample of 101 stars, between 3-500 million years old, were observed in deep exposures with a coronagraph to search for faint sub-stellar companions. A total of 288 candidate companions were discovered around the sample stars, which were re-imaged at subsequent epochs to determine physical association with the candidate host stars by checking for common proper motion. Benefitting from a highly accurate astrometric calibration of the observations, we were able to successfully apply the common proper motion test in the majority of the cases, including stars with proper motions as small as 20 milli-arcseconds/year. The results from the survey include the discovery of three new brown dwarf companions (HD 49197B, HD 203030B, and ScoPMS 214B), 43 new stellar binaries, and a triple system. The physical association of an additional, a priori-suspected, candidate sub-stellar companion to the star HII 1348 is astrometrically confirmed. The newly-discovered and confirmed young brown dwarf companions span a range of spectral types between M5 and T0.5, and will be of prime significance for constraining evolutionary models of young brown dwarfs and extra-solar planets. Based on the 3 new detections of sub-stellar companions in the 101 star sub-sample and following a careful estimate of the survey incompleteness, a Bayesian statistical analysis shows that the frequency of 0.012-0.072 solar-mass brown dwarfs in 30-1600 AU orbits around young solar analogs is 6.8% (-4.9%, +8.3%; 2-sigma limits). While this is a factor of 3 lower than the frequency of stellar companions to G-dwarfs in the same orbital range, it is significantly higher than the frequency of brown dwarfs in 0-3 AU orbits discovered through precision radial velocity surveys. It is also fully consistent with the observed frequency of 0-3 AU extra-solar planets. Thus, the result demonstrates that the radial-velocity "brown dwarf desert" does not extend to wide separations, contrary to previous belief.
Le spectre solaire de 2,8 à 23,7 microns: Measures and identifications; with comments on the spectra of telluric H20 and CO2 as observed in the solar spectrum, 2.8
Author: Marcel Migeotte
Publisher:
ISBN:
Category : Spectrum, Solar
Languages : en
Pages : 170
Book Description
Publisher:
ISBN:
Category : Spectrum, Solar
Languages : en
Pages : 170
Book Description
The President's Report to the Board of Regents for the Academic Year ...
Author: University of Michigan
Publisher:
ISBN:
Category :
Languages : en
Pages : 1100
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages : 1100
Book Description
Report to the Board of Regents ...
Author: University of Michigan
Publisher:
ISBN:
Category :
Languages : en
Pages : 476
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages : 476
Book Description
Catalog of Copyright Entries. Third Series
Author: Library of Congress. Copyright Office
Publisher: Copyright Office, Library of Congress
ISBN:
Category : Copyright
Languages : en
Pages : 1672
Book Description
Includes Part 1, Number 1 & 2: Books and Pamphlets, Including Serials and Contributions to Periodicals (January - December)
Publisher: Copyright Office, Library of Congress
ISBN:
Category : Copyright
Languages : en
Pages : 1672
Book Description
Includes Part 1, Number 1 & 2: Books and Pamphlets, Including Serials and Contributions to Periodicals (January - December)