3 edition of The winds of B supergiants [STX task 3400-001) found in the catalog.
The winds of B supergiants [STX task 3400-001)
by National Aeronautics and Space Administration, National Technical Information Service, distributor in [Washington, DC, Springfield, Va
Written in English
|Statement||[authors, D. Massa, A.W. Fullerton, R.K. Prinja].|
|Series||[NASA contractor report] -- CR-206871., NASA contractor report -- NASA CR-206871.|
|Contributions||Fullerton, A. W., Prinja, R. K., United States. National Aeronautics and Space Administration.|
|The Physical Object|
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Abstract: This work presents a homogeneous derivation of atmospheric parameters and iron abundances for a sample of giant and subgiant stars which host giant planets, as well as a control sample of subgiant stars not known to host giant planets. The analysis is done using the same technique as for our previous analysis of a large sample of planet-hosting and control sample dwarf by: Okay, so Activision has just updated the official website with some new information and the digging operation had to commence. Basically, Toys For Bob is now credited for their development support and porting the game, alongside Iron Galaxy Studios being mentioned for their effort on the porting (unknown exactly which version of the remakes, but.
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Get this from a library. The winds of B supergiants [STX task ). [Derck Louis Massa; A W Fullerton; R K Prinja; United States. National Aeronautics and Space Administration.]. Anual Report: The Winds of B Supergiants (STX Task ) As outlined in the proposal, the first step in this project was the analysis of the time series of 2 B supergiants and an O star (the "MEGA 2" data).
These data were analyzed and reported on at the ESO workshop "Cyclical Variability in Stellar Winds". Get this from a library. An[n]ual report: the winds of B supergiants [STX task ).
[A W Fullerton; United States. National Aeronautics and Space Administration.;]. The Winds of B Supergiants (STX Task ) During the first quarter of this contract, work concentrated primarily on data acquisition and reduc-tion.
As outlined in the proposal, the first step in this project was the analysis of the time series of 2 B supergiants and an O star (the "MEGA 2" data).
Investigating the 3D Structure of the Winds of Hot Supergiants. NASA Astrophysics Data System (ADS) Klement, Robert. An observational effort targeting supergiant stars of spectral classes B and A has been started using the VEGA high spectral resolution visible beam combiner at the CHARA array.
The H-alpha emission from the structured stellar winds was resolved with respect to the. Abstract: Extremely broad emission wings at H$\beta$ and H$\alpha$ have been found in VFTS data for five very luminous BA supergiants in or near 30 Doradus in the Large Magellanic Cloud. The profiles of both lines are extremely asymmetrical, which we have found to be caused by very broad diffuse interstellar bands (DIBs) in the longward wing of H$\beta$ and the shortward wing of H$\alpha$.
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(Technical Monitor) We present the most suitable data sets available in the International Ultraviolet Explorer (IUE) archive for the study of time-dependent stellar winds in early B supergiants. The UV line profile variability in 11 B0 to B3.
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explanation blue bibcodes open ADS page with paths to full text Author name code: foing ADS astronomy entries on author:"Foing, Bernard H." Title: Food for Extra-Terrestrial Astronaut Missions on Native Soil Authors: Pouwels, C.
R.; Wamelink, G. W.; Musilova, M.; Foing, B. LPIP Altcode: Food demand during extra-terrestrial missions is of high importance. This report summarizes the progress of the work conducted under the program "The Winds of B Supergiants," conducted by Raytheon STX Corporation.
The report consists of a journal article "Wind variability in B supergiants III. Corotating spiral structures in the stellar wind of HD " The first step in the project was the analysis of the.
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Spectral scans at approximately A resolution have been obtained in the far-ultraviolet of eight stars which have high mass-loss rates from stellar P Cygni characteristics of the line profiles appear to vary inversely as the mass flow rate, and in P Cygni.
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