Milliarcsecond resolution infrared observations of young stars in Taurus and Ophiuchus

1987 ◽  
Vol 320 ◽  
pp. 344 ◽  
Author(s):  
M. Simon ◽  
R. R. Howell ◽  
A. J. Longmore ◽  
B. A. Wilking ◽  
D. M. Peterson ◽  
...  

2005 ◽  
Vol 618 (2) ◽  
pp. 795-809 ◽  
Author(s):  
Theodore Simon ◽  
S. E. Dahm


1987 ◽  
Vol 115 ◽  
pp. 71-74
Author(s):  
H. Zinnecker ◽  
A. Chelli ◽  
C. Perrier

High spatial resolution infrared observations (mostly at L, some at K) of several young stars in the ρ Oph dark cloud were obtained with the specklegraph at the ESO 3.6m telescope in Chile in July 1985. Sources included EL29, EL21, EL14 and EL9 (Elias 1978, Table 2), and were all measured in two orthogonal directions, W-E (PA=90°) and N-S (PA=180°). Here we shall present visibility functions for EL29 and EL21 and indicate the spatial structure and dimension of these objects. We refer to Elias (1978, p.468/69) for earlier studies of EL29 and EL21.





1991 ◽  
Vol 147 ◽  
pp. 289-292
Author(s):  
Klaus-Werner Hodapp ◽  
John Rayner ◽  
Hua Chen

Clusters of young stars have been found near a number of compact HII regions. These clusters do not show a turnover in the K-band luminosity and are probably several million years old. In L 1641 only moderate clustering tendency has been observed and many sources show signs of extremely young age.



2013 ◽  
Vol 552 ◽  
pp. A14 ◽  
Author(s):  
H. Ohlendorf ◽  
T. Preibisch ◽  
B. Gaczkowski ◽  
T. Ratzka ◽  
J. Ngoumou ◽  
...  


1999 ◽  
Vol 521 (2) ◽  
pp. L129-L132 ◽  
Author(s):  
Ray Jayawardhana ◽  
Lee Hartmann ◽  
Giovanni Fazio ◽  
R. Scott Fisher ◽  
Charles M. Telesco ◽  
...  




1979 ◽  
Vol 229 ◽  
pp. 990 ◽  
Author(s):  
P. M. Harvey ◽  
M. F. Campbell ◽  
W. F. Hoffmann ◽  
H. A., Jr. Thronson ◽  
I. Gatley


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