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Wednesday, December 2, 2020 | History

2 edition of high-dispersion spectral analysis of the Ba II star HD 204075 (Capricorni) found in the catalog.

high-dispersion spectral analysis of the Ba II star HD 204075 (Capricorni)

Jack L Tech

high-dispersion spectral analysis of the Ba II star HD 204075 (Capricorni)

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Published by U.S. Govt. Print. Off. in Washington .
Written in English

    Subjects:
  • Stars -- Spectra

  • Edition Notes

    SeriesNational Bureau of Standards monograph -- 119, NBS monograph -- 119
    The Physical Object
    Paginationvi, 170 p.
    Number of Pages170
    ID Numbers
    Open LibraryOL18168389M


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high-dispersion spectral analysis of the Ba II star HD 204075 (Capricorni) by Jack L Tech Download PDF EPUB FB2

High-dispersion spectral analysis of the Ba II star HD (Capricorni). Washington, U.S. Govt. Print. Off., (OCoLC) Material Type: Government publication, National government publication: Document Type: Book: All Authors / Contributors: Jack L Tech.

Buy A high-dispersion spectral analysis of the Ba II star HD (Capricorni) (National Bureau of Standards monograph) on FREE SHIPPING on qualified orders. Technical Report: A HIGH-DISPERSION SPECTRAL ANALYSIS OF THE Ba II STAR HD (zeta CAPRICORNI).

A High-Dispersion Spectral Analysis of the Ba II Star HD (Capricorni) (National Bureau of Standards Monograph, ): Books - at: Hardcover. Buy A High-Dispersion Spectral Analysis of the Ba II Star HD (Capricorni) (National Bureau of Standards Monograph, ) by Jack L Tech (ISBN:) from Amazon's Book Store.

Everyday low prices and free delivery on eligible : Jack L Tech. Part of the Astronomy and Astrophysics Abstracts book series A high-dispersion spectral analysis of the Ba II star HD (3- Capricorni).

Bull. American Astron. Soc., Vol. 1, – (). Abstr. AAS. The expected fraction of evolved close binaries among main-sequence stars of spectral type earlier than A5.

Astron. Journ. We present high dispersion (R ∼ 16,) optical ( − ˚A) spectra of stars obtained with the Palomar inch Telescope.

The majority of stars observed are part of the Spitzer Legacy Science Program The Formation& Evolu-tion of Planetary Systems. Through detailed analysis we determine stellar prop. () High-Dispersion Spectroscopy of the B[e] Supergiants S In: Davidson K., Moffat A.F.J., Lamers H.J.G.L.M.

(eds) Physics of Luminous Blue Variables. Astrophysics and Space Science Library (A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Cited by: 1.

For our study we choose the B[e] star HD of the FS CMa type because of the indication that this star is a post-main-sequence star, although still not highly evolved. Therefore, it can be a good object for testing evolutionary models. Currently, HD is the most extensively observed FS CMa star which makes it an ideal object for modelling.

Abstract: We present high-dispersion (R~16,) optical ( A) spectra of stars obtained with the Palomar 60 inch telescope. The majority of stars observed are part of the Spitzer Legacy Science Program "The Formation and Evolution of Planetary Systems." Through detailed analysis we determine stellar properties for this sample, including radial and rotational.

sequence, Be star LS with a radius of 6R⊙. PSR B−63 is a middle-aged pulsar ( kyr) with a relatively short period of 48 ms. Its average DM is about pc cm−3. The system is an eccentric binary (e = ) with an orbital period of yr and a projected semi-major axis,asini, of light seconds ( AU).

Compra A High-Dispersion Spectral Analysis of the Ba II Star HD (Capricorni) (National Bureau of Standards Monograph, ).

SPEDIZIONE GRATUITA su ordini idoneiFormat: Copertina rigida. This page is organized by the McCook and Sion () WD number for each star. Clicking on the WD number will lead to a list of processed spectra for that star.

That list identifies individual processed NEWSIPS spectra for the selected star (by SWP number) and also any coadded spectra which were produced.

Noté /5. Retrouvez A High-Dispersion Spectral Analysis of the Ba II Star HD (Capricorni) (National Bureau of Standards Monograph, ) et des millions de livres en stock sur Achetez neuf ou d'occasionFormat: Relié.

On March we conducted a campaign with the Hubble Space Telescope GHRS to observe the Si IV λλ, lines of the Be star γ. A High-Dispersion Spectral Analysis of the Ba II Star HD Capricorni [National Bureau of Standards, Monograph ] | Jack L Tech | ISBN: | Kostenloser Versand für alle Bücher mit Versand und Verkauf duch : Gebundenes Buch.

Full text of "Bibliography on atomic transition probabilities ( through October )" See other formats. Tables of Spectral-Line Intensities Part I - Arranged by Elements-[2nd]-[William F Meggers, Charles H Corliss, Bourdon F Scribner],Parti National Bureau of Standards DEPARTMENT Of / U.& Tables of Spectral-Line Intensities Arranged by Elements W, F.

Meggers prepares to measure one of the spectrograms on which these tables of spectral line intensities. Full text of "Publications of the National Bureau of Standards Catalog" See other formats.