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20230706230849.2 |
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|a (TOE)ost6691692
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|a (TOE)6691692
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|a TOE
|c TOE
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|a GDWR
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|a 71
|2 edbsc
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|a E 1.99: conf-9005248--4
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|a E 1.99:la-ur-90-2374
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|a conf-9005248--4
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| 088 |
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|a la-ur-90-2374
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| 245 |
0 |
4 |
|a The impact of IUE on studies of the nova outburst
|h [electronic resource] :
|b 1986--1990.
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| 260 |
|
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|a Washington, D.C. :
|b United States. Department of Energy ;
|a Oak Ridge, Tenn. :
|b distributed by the Office of Scientific and Technical Information, U.S. Department of Energy,
|c 1990.
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| 300 |
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|a Pages: (34 p) :
|b digital, PDF file.
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| 336 |
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|a text
|b txt
|2 rdacontent.
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| 337 |
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|a computer
|b c
|2 rdamedia.
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| 338 |
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|a online resource
|b cr
|2 rdacarrier.
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| 500 |
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|a Published through SciTech Connect.
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| 500 |
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|a 01/01/1990.
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| 500 |
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|a "la-ur-90-2374"
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| 500 |
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|a " conf-9005248--4"
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| 500 |
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|a "DE90014915"
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| 500 |
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|a Evolution in astrophysics: IUE astronomy in the era of new space missions, Toulouse (France), 29 May - 1 Jun 1990.
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| 500 |
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|a Starrfield, S.
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| 520 |
3 |
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|a In this review I will concentrate on the improvements in our understanding of the nova outburst that have occurred since the IUE meetings in London in 1986 and Goddard in 1988 and those results that have occurred as a direct result of studies with the IUE satellite. These involve the four outbursts that have occurred in the LMC, the numerous recurrent novae outbursts, and a number of archival studies. As a direct result of IUE studies done since 1986, we can now state that fast novae become super-Eddington at maximum, that many novae decline at the same rate, and that neon novae may be more numerous than thought previously. In addition, we have found that there are differences in the outburst characteristics between novae with giant secondaries and those with compact secondaries. 18 refs., 11 figs., 1 tab.
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| 536 |
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|b W-7405-ENG-36.
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| 650 |
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7 |
|a Novae.
|2 local.
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| 650 |
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7 |
|a Ultraviolet Spectra.
|2 local.
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| 650 |
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7 |
|a Bolometers.
|2 local.
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| 650 |
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7 |
|a Luminosity.
|2 local.
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| 650 |
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|a Red Giant Stars.
|2 local.
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|a Satellites.
|2 local.
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|a Eruptive Variable Stars.
|2 local.
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|a Giant Stars.
|2 local.
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|a Measuring Instruments.
|2 local.
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7 |
|a Optical Properties.
|2 local.
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| 650 |
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|a Physical Properties.
|2 local.
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| 650 |
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7 |
|a Spectra.
|2 local.
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| 650 |
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7 |
|a Stars.
|2 local.
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| 650 |
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7 |
|a Variable Stars.
|2 local.
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| 650 |
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7 |
|a Classical And Quantum Mechanics, General Physics.
|2 edbsc.
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| 710 |
2 |
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|a Los Alamos National Laboratory.
|4 res.
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| 710 |
1 |
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|a United States.
|b Department of Energy.
|4 spn.
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| 710 |
1 |
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|a United States.
|b Department of Energy.
|b Office of Scientific and Technical Information.
|4 dst.
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| 856 |
4 |
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|u http://www.osti.gov/scitech/biblio/6691692
|z Online Access
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| 907 |
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|a .b59801116
|b 03-06-23
|c 05-26-10
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| 998 |
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|a web
|b 09-09-16
|c f
|d m
|e p
|f eng
|g
|h 4
|i 3
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|a Information bridge
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|i be08001b-ab08-5e96-aab9-e0b66076ad0c
|s 05054733-3d0b-5016-9b0b-a94ec9545367
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| 952 |
f |
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|p Can circulate
|a University of Colorado Boulder
|b Online
|c Online
|d Online
|e E 1.99: conf-9005248--4
|h Superintendent of Documents classification
|i web
|n 1
|
