The circumstellar gas surrounding 51 Ophiuchi - A candidate proto-planetary system similar to Beta Pictoris

1993 ◽  
Vol 402 ◽  
pp. L61 ◽  
Author(s):  
C. A. Grady ◽  
J. M. S. Silvis
1991 ◽  
Vol 377 ◽  
pp. L49 ◽  
Author(s):  
A. Boggess ◽  
Frederick C. Bruhweiler ◽  
C. A. Grady ◽  
Dennis C. Ebbets ◽  
Yoji Kondo ◽  
...  

1999 ◽  
Vol 172 ◽  
pp. 313-316
Author(s):  
Pawel Artymowicz

AbstractThe past decade brought direct evidence of the previously surmised exoplanetary systems. A variety of planetary system types exist those around pulsars, around both young and old main-sequence stars (as evidenced by planetesimal disks of the Beta Pictoris-type), and the mature giant exoplanets found in radial velocity surveys. The surprising diversity of the exoplanetary systems is addressed by several theories of their origin.


1989 ◽  
Vol 120 ◽  
pp. 221-226
Author(s):  
Francesco Paresce ◽  
Pawel Artymowicz

SummaryWe summarize the observed properties and deduced physical characteristics of the Beta Pictoris circumstellar nebula obtained from a detailed analysis of existing IR and optical data. On the basis of these results, we reject the hypothesis that the observed feature is a bipolar nebula surrounding an evolved star. We claim the nebula is a flattened disk of orbiting particles making up a planetary system in its clearing out phase as small grains collide, erode, and are swept out by radiation pressure.


1988 ◽  
Vol 20 (1) ◽  
pp. 693-701
Author(s):  
F. D. Drake ◽  
George Marx ◽  
N. D. Papagiannis ◽  
R. D. Brown ◽  
P. Connes ◽  
...  

The past three years have seen not only a growth in the activities of our commission, but an extension of its activities into important areas which have heretofore motivated too little activity. Of particular interest have been the many activities directed towards elucidating the question of the abundance of extrasolar planetary systems. There have been a number of observations showing the presence of disks of dust around nearby stars, disks which fit the idea that stars are often formed with an accompanying disk of dust which may in many or perhaps all cases produce a planetary system. Infra-red evidence for dust disks exists for something like twenty stars. The disk of Beta Pictoris has even been clearly imaged at optical wavelengths, showing without a doubt that such disk structures exist. One very impressive detection of an apparent brown dwarf object has also been made; should this be confirmed by other observations, it would be clear evidence for the existence of planet-like bodies in the systems of other stars.


1987 ◽  
Vol 92 ◽  
pp. 526-528
Author(s):  
F.C. Bruhweiler ◽  
Y. Kondo

Continued UV monitoring at high spectral resolution utilizing the International Ultraviolet Explorer (IUE) of the IRAS candidate proto-planetary system, Beta Pictoris (Also see Kondo and Bruhweiler 1985; and references cited therein.), has revealed two components to the circumstellar absorption. The first is a stable absorption component at or near the stellar photospheric velocity, possibly arising from gas orbiting in a gaseous disk, while the second component represents strong variable excess absorption sometimes extending up to +200 km s-1. The variability of this second component accounts for most of the spectral variability observed in Beta Pic. Variable circumstellar absorption observed in the resonance lines and UV62 and 63 multiplets of Fe II reveal an episode of mass inflow which lasted over a period of 12 to 13 months (see Fig. 1).


1991 ◽  
Vol 371 ◽  
pp. L27 ◽  
Author(s):  
Frederick C. Bruhweiler ◽  
C. A. Grady ◽  
Yoji Kondo

1986 ◽  
Author(s):  
Harold Masursky ◽  
Kaare Aksnes ◽  
G.E. Hunt ◽  
M.Y. Marov ◽  
P.M. Millman ◽  
...  

Author(s):  
Karel Schrijver

This chapter describes how the first found exoplanets presented puzzles: they orbited where they should not have formed or where they could not have survived the death of their stars. The Solar System had its own puzzles to add: Mars is smaller than expected, while Venus, Earth, and Mars had more water—at least at one time—than could be understood. This chapter shows how astronomers worked through the combination of these puzzles: now we appreciate that planets can change their orbits, scatter water-bearing asteroids about, steal material from growing planets, or team up with other planets to stabilize their future. The special history of Jupiter and Saturn as a pair bringing both destruction and water to Earth emerged from the study of seventeenth-century resonant clocks, from the water contents of asteroids, and from experiments with supercomputers imposing the laws of physics on virtual worlds.


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