scholarly journals Mid-infrared interferometry of massive young stellar objects

2008 ◽  
Vol 131 ◽  
pp. 012024 ◽  
Author(s):  
H Linz ◽  
B Stecklum ◽  
R Follert ◽  
Th Henning ◽  
R van Boekel ◽  
...  
Author(s):  
J. Varga ◽  
P. Ábrahám ◽  
Th. Ratzka ◽  
J. Menu ◽  
K. Gabányi ◽  
...  

AbstractWe present our approach of visibility modeling of disks around low-mass (< 2 M⊙) young stellar objects (YSOs). We compiled an atlas based on mid-infrared interferometric observations from the MIDI instrument at the VLTI. We use three different models to fit the data. These models allow us to determine overall sizes (and the extent of the inner gaps) of the modeled circumstellar disks.


2009 ◽  
Vol 505 (2) ◽  
pp. 655-661 ◽  
Author(s):  
H. Linz ◽  
Th. Henning ◽  
M. Feldt ◽  
I. Pascucci ◽  
R. van Boekel ◽  
...  

2010 ◽  
Vol 522 ◽  
pp. A17 ◽  
Author(s):  
R. Follert ◽  
H. Linz ◽  
B. Stecklum ◽  
R. van Boekel ◽  
Th. Henning ◽  
...  

2012 ◽  
Vol 8 (S287) ◽  
pp. 280-281
Author(s):  
Olga Bayandina ◽  
Irina Val'tts ◽  
Grigorii Larionov

AbstractAn identification has been conducted of class I methanol masers with 1) short-wave infrared objects EGO (extended green objects) - tracer bipolar outflow of matter in young stellar objects, and 2) isolated pre-protostellar gas-dust cores of the interstellar medium which are observed in absorption in the mid-infrared in the Galactic plane. It is shown that more than 50% of class I methanol masers are identified with bipolar outflows, considering the EGO as bipolar outflows (as compared with the result of 22% in the first version of the MMI catalog that contains no information about EGO). 99 from 139 class I methanol masers (71%) are identified with SDC. Thus, it seems possible that the MMI can be formed in isolated self-gravitating condensations, which are the silhouette of dark clouds - IRDC and SDC.


2003 ◽  
Vol 126 (5) ◽  
pp. 2411-2420 ◽  
Author(s):  
C. L. Barbosa ◽  
A. Damineli ◽  
R. D. Blum ◽  
P. S. Conti

2012 ◽  
Vol 201 (2) ◽  
pp. 11 ◽  
Author(s):  
Á. Kóspál ◽  
P. Ábrahám ◽  
J. A. Acosta-Pulido ◽  
C. P. Dullemond ◽  
Th. Henning ◽  
...  

2009 ◽  
Vol 5 (H15) ◽  
pp. 734-734
Author(s):  
John R. Stauffer ◽  
Maria Morales ◽  
Luisa Rebull

In Morales et al. (2009), we have recently investigated the mid-infrared (3.6 to 8.0 micron) variability of young-stellar objects (YSOs) using the IRAC camera on the Spitzer Space Telescope. Specifically, we obtained synoptic photometry of about 70 YSOs in the ~1 Myr old IC1396A globule over a 14 day period. More than half of the YSOs were detectably variable, with amplitudes up to about 0.2 magnitudes. About a third of these objects showed quasi-sinusoidal light curves with apparent periods of typically 5 to 12 days. At least two families of models can explain such light curves: (a) a Class II YSO with a photospheric hot spot which locally heats the inner circumstellar disk which is viewed from slightly above the disk plane, and (b) a YSO with a warped disk or with some other non-axisymmetric inner disk density profile, also seen with a view angle slightly above the disk plane. The two models can both yield light curve shapes and amplitudes similar to what we observe in the mid-infrared, but produce very different light curves at shorter wavelengths dominated by the stellar photosphere. Because we only had IRAC photometry for IC1396A, we were not able to discriminate between the two models for this set of data.


Sign in / Sign up

Export Citation Format

Share Document