scholarly journals A Disk Census for the Nearest Group of Young Stars: Mid-Infrared Observations of the TW Hydrae Association

1999 ◽  
Vol 521 (2) ◽  
pp. L129-L132 ◽  
Author(s):  
Ray Jayawardhana ◽  
Lee Hartmann ◽  
Giovanni Fazio ◽  
R. Scott Fisher ◽  
Charles M. Telesco ◽  
...  
2021 ◽  
Author(s):  
Arrate Antunano ◽  
Leigh N Fletcher ◽  
Glenn S Orton ◽  
Henrik Melin ◽  
Padraig T. Donnelly ◽  
...  

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.


2001 ◽  
Vol 205 ◽  
pp. 224-227
Author(s):  
Jean L. Turner

Subarcsecond radio and infrared observations reveal a class of luminous, obscured, optically thick HII regions associated with extremely large young clusters in nearby starburst galaxies. VLA images show bright radio nebulae with ne ∼ 104 cm−3, densities characteristic of young Galactic compact HII regions. Excitation of the nebulae requires the presence of several thousand O stars within regions of 1-10 pc extent, corresponding to clusters containing 105–106 stars. The compact nebulae are also bright in the mid-infrared, and can for significant fractions of not only the total IR luminosity, but also the total bolometric luminosity, of the parent galaxies. The prototype for these “supernebulae” is the large, obscured cluster in the dwarf galaxy NGC 5253.


1997 ◽  
Vol 163 ◽  
pp. 799-800
Author(s):  
Craig H. Smith ◽  
Christopher M. Wright ◽  
David K. Aitken ◽  
Patrick F. Roche

AbstractWe present the results from mid-infrared spectro-polarimetric observations of a number of bi-polar outflow sources. The specto-polarimetric data provides information on the polarization mechanism and the magnetic field direction. The field direction in the disks of the observed sources is most often normal to the ambient field direction and lies in the plane of the disk, indicating a toroidal rather than poloidal field configuration.


2005 ◽  
Vol 130 (5) ◽  
pp. 2237-2240 ◽  
Author(s):  
J. Farihi ◽  
B. Zuckerman ◽  
E. E. Becklin

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

2006 ◽  
Vol 648 (1) ◽  
pp. L25-L28 ◽  
Author(s):  
L. Snijders ◽  
P. P. van der Werf ◽  
B. R. Brandl ◽  
S. Mengel ◽  
D. Schaerer ◽  
...  

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