The Near-Ultraviolet Continuum of Late-Type Stars

2000 ◽  
Vol 119 (5) ◽  
pp. 2445-2454 ◽  
Author(s):  
Carlos Allende Prieto ◽  
David L. Lambert
2014 ◽  
Vol 797 (1) ◽  
pp. 69 ◽  
Author(s):  
Ian U. Roederer ◽  
Heather R. Jacobson ◽  
Thanawuth Thanathibodee ◽  
Anna Frebel ◽  
Elizabeth Toller

1980 ◽  
Vol 5 ◽  
pp. 263-276 ◽  
Author(s):  
A. K. Dupree

A vast increase in the amount of information on cool stars has occurred during the past 3 years starting with the spectroscopy of the brightest objects from the Princeton experiment on Copernicus, the near ultraviolet balloon measurements from BUSS, low dispersion observations in the far ultraviolet from rocket instruments, and most recently, spectra from the International Ultraviolet Explorer satellite (IUE). IUE now gives access to a wide variety of cool stars and stellar systems enabling systematic studies to be made.Drawing on the most recent material from IUE, we discuss the presence and structure of chromospheres and coronae in single stars of varying gravities, surface temperatures, and activity. Evidence of mass loss and the concurrent presence of a corona are also noted. Binary systems of late-type stars (the RS CVn and W UMa type) are briefly discussed since they display extremes of surface activity. A binary system such as VV Cep containing a late-type star and an early-type companion provides a unique probe of cool extended stellar atmospheres.


2009 ◽  
Vol 691 (2) ◽  
pp. 1634-1647 ◽  
Author(s):  
C. Ian Short ◽  
P. H. Hauschildt
Keyword(s):  

2019 ◽  
Vol 871 (2) ◽  
pp. 167 ◽  
Author(s):  
Adam F. Kowalski ◽  
John P. Wisniewski ◽  
Suzanne L. Hawley ◽  
Rachel A. Osten ◽  
Alexander Brown ◽  
...  

1989 ◽  
Vol 134 ◽  
pp. 385-386
Author(s):  
Thomas J. Balonek ◽  
Paul A. Heckert ◽  
Richard Elston ◽  
Paul S. Smith ◽  
Michael L. Sitko

We have observed a period of rapid and intense optical-infrared brightness and polarization variability in the quasar 3C 279. The observations were obtained as part of an ongoing study of the optical-infrared continuum evolution in a sample of optically violent variable (OVV) quasars and BL Lacertae objects. Simultaneous broadband UBVRI photometric and polarimetric observations are used to study the optical continuum spectral evolution and wavelength dependent linear polarization and to search for broad near-ultraviolet continuum spectral components.


1997 ◽  
Vol 161 ◽  
pp. 707-709 ◽  
Author(s):  
Jun Jugaku ◽  
Shiro Nishimura

AbstractWe continued our search for partial (incomplete) Dyson spheres associated with 50 solar-type stars (spectral classes F, G, and K) within 25 pc of the Sun. No candidate objects were found.


2002 ◽  
Vol 4 ◽  
pp. 393-393
Author(s):  
A. Boselli ◽  
J. Lequeux ◽  
G. Gavazzi
Keyword(s):  

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