X-ray flare characteristics in lambda Eridani (ROSAT)
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X-ray flare characteristics in lambda Eridani (ROSAT) final report for NASA contract S-57776-F by

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Published by National Aeronautics and Space Administration, National Technical Information Service, distributor in [Washington, DC, Springfield, Va .
Written in English

Subjects:

  • B stars.,
  • Variable stars.,
  • X rays.,
  • Stellar flares.

Book details:

Edition Notes

StatementMyron A. Smith.
Series[NASA contractor report] -- NASA-CR-204076., NASA contractor report -- NASA CR-204076.
ContributionsUnited States. National Aeronautics and Space Administration.
The Physical Object
FormatMicroform
Pagination1 v.
ID Numbers
Open LibraryOL18131616M

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Final report for on task (SP) entitled "X-ray flare characteristics in lambda Eridani" X-Ray Flare Characteristics in lambda Eridani. By Myron A. Smith. Abstract. The X-ray component consisted of observations from both the ASCA and ROSAT satellites Topics: Space Radiation. Year: OAI identifier: oai:   X-ray flaring from ROSAT observations in The X-ray component consisted of observations from both ROSAT (subject of this task) and ASCA satellites. The flare event observed by ROSAT caught the astronomical hot star community by surprise because X-ray flares have not been observed from other single B-type stars, before or :// A giant X-ray flare on Lambda Eridani (B2e) Authors: Smith, Myron A.; , can be fitted well to a Raymond-Smith temperature parameter of 14 MK and luminosity 4 x 10 exp 31 ergs/s; these are characteristics of giant stellar flares. With an estimated duration of ab s, this event is arguably the strongest X-ray flare yet observed LS.

  Final Report for on Task (SP) entitled: "X-Ray Flare Characteristics in lambda Eridani" (ASCA) Myron A. Smith, CSC/Science Programs This proposal was for a joint X-rayultravioletground-based study of the abnormal Be star lambda Eri, which has previously shown evidence of X-ray flaring from ROSAT observations in Artificial intelligence in clinical research. X-Ray Flare Characteristics in the B2e Star Lambda Eridani (ROSAT) April /_Artificial_intelligence_in_clinical_research.   STARS and STARS OF THE WEEK Star Count: Created by Jim Kaler, Prof. Emeritus of Astronomy, University of Illinois Learn about stellar spectra in STARS AND THEIR SPECTRA: An Introduction to the Spectral Sequence, Second Ed., with two new chapters and new illustrations, Cambridge University Press (UK or North America), From the Sun to the Stars: the OLLI   Uma estrela eruptiva é uma estrela variável que pode passar por aumentos dramáticos e imprevisíveis no seu brilho por alguns minutos. Acredita-se que, assim como as erupções solares, as dessas estrelas se devam à energia magnética armazenada na atmosfera das mesmas. O aumento de brilho ocorre, no espectro eletromagnético, desde raios-X até ondas de ://

X-Ray Flare Characteristics in the B2e Star Lambda Eridani (ROSAT) We have made three ROSAT HRI observations of the Orion Nebula region, ranging in exposure time from ~ 10 to ~ 50 ksecs. /_ROSAT_HRI_Observations_of_the_Orion_Nebula.   Within the Multimedia Gallery section you will find sets of images relating to: Scientific results (real images, artistic representations, animations, etc.). Institutional events (meetings, educational activities, etc.). Facilities and instrumentation of the IAC and the Observatorios de Canarias;   Bibliography Myron Smith Buta, R. J. and Smith, M. A. , "The Light Variations of Nonradial Pulsations. I. Theory and Application to Line Profile Variations ~msmith/ "Discovery of a variable supersoft X-ray source in the Large Magellanic Cloud during the ROSAT All-Sky Survey," Astronomy and Astrophysics, , , L9-L Schelgel, E.M.; Petre, R.; July "A ROSAT upper limit on X-ray emission from SN A," Astrophysical Journal, Part 2 - Letters, , 1, LL