Cycles of Variability in Jupiter's Atmosphere from Ground-Based Mid-Infrared Observations

2021 ◽  
Author(s):  
Arrate Antunano ◽  
Leigh N Fletcher ◽  
Glenn S Orton ◽  
Henrik Melin ◽  
Padraig T. Donnelly ◽  
...  
Keyword(s):  
Mid Infrared ◽  
Infrared Observations

scholarly journals The Youngest Star-Forming Regions in Galaxies: Giant Compact HII Regions and Protoglobular Clusters?

2001 ◽  
Vol 205 ◽  
pp. 224-227
Author(s):  
Jean L. Turner
Keyword(s):  
Dwarf Galaxy ◽  
Hii Regions ◽  
Starburst Galaxies ◽  
Mid Infrared ◽  
Infrared Observations ◽  
Star Forming ◽  
Bolometric Luminosity ◽  
Star Forming Regions ◽  
Young Clusters ◽  
Compact Hii Regions

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.

scholarly journals Mid-infrared Observations of Magnetic Fields in the Disks of Bi-Polar Outflow Sources

1997 ◽  
Vol 163 ◽  
pp. 799-800
Author(s):  
Craig H. Smith ◽  
Christopher M. Wright ◽  
David K. Aitken ◽  
Patrick F. Roche
Keyword(s):  
Magnetic Field ◽  
Magnetic Fields ◽  
Field Configuration ◽  
Field Direction ◽  
Magnetic Field Direction ◽  
Poloidal Field ◽  
Mid Infrared ◽  
Infrared Observations ◽  
Polarization Mechanism ◽  
The Magnetic Field

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.

scholarly journals Mid-Infrared Observations of the White Dwarf-Brown Dwarf Binary GD 1400

2005 ◽  
Vol 130 (5) ◽  
pp. 2237-2240 ◽  
Author(s):  
J. Farihi ◽  
B. Zuckerman ◽  
E. E. Becklin
Keyword(s):  
White Dwarf ◽  
Brown Dwarf ◽  
Mid Infrared ◽  
Infrared Observations

scholarly journals Subarcsecond Resolution Mid-Infrared Observations of Super Star Clusters in the Antennae (NGC 4038/4039)

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

scholarly journals Local luminous infrared galaxies: Spatially resolved mid-infrared observations with Spitzer/IRS

2010 ◽  
Vol 45 (1) ◽  
pp. 99-111 ◽  
Author(s):  
Almudena Alonso-Herrero ◽  
Miguel Pereira-Santaella ◽  
George H. Rieke ◽  
Luis Colina ◽  
Charles W. Engelbracht ◽  
...  
Keyword(s):  
Infrared Galaxies ◽  
Mid Infrared ◽  
Infrared Observations ◽  
Luminous Infrared Galaxies ◽  
Spatially Resolved

A method for reducing atmospheric noise without chopping for ground-based mid-infrared observations

2016 ◽  
Author(s):  
Tomohiko Nakamura ◽  
Takashi Miyata ◽  
Shigeyuki Sako ◽  
Takafumi Kamizuka ◽  
Kentaro Asano ◽  
...  
Keyword(s):  
Mid Infrared ◽  
Infrared Observations ◽  
Atmospheric Noise

scholarly journals UCHII regions in the Antennae

2006 ◽  
Vol 2 (S237) ◽  
pp. 476-476
Author(s):  
L. Snijders ◽  
L. J. Kewley ◽  
P. P. van der Werf ◽  
B. R. Brandl
Keyword(s):  
Emission Line ◽  
Spatial Resolution ◽  
Average Density ◽  
Physical Characteristics ◽  
Stellar Clusters ◽  
Mid Infrared ◽  
Infrared Observations ◽  
Star Forming ◽  
Compact Material ◽  
Star Forming Regions

AbstractWe explore the physical characteristics of young stellar clusters in the Antennae by combining recent ground- and space-based mid-infrared observations with a newly developed set of diagnostic diagrams. Spitzer data give an overview of the star-forming regions extending over hundreds of parsecs, showing a dominant diffuse ISM component with a density of 102 cm−3 plus a small fraction of very compact material (106 cm−3). With its higher spatial resolution VISIR gives a close-up view of the latter component. Its emission line ratios suggest that these regions are fundamentally different from local star-forming regions. Instead of having small isolated UCHII regions, as in local star-forming regions, the average density of the medium of the whole region falls in the (ultra)compact regime, exceeding 104 cm−3 over tens of parsecs.

scholarly journals High Spatial Resolution Mid-Infrared Observations of Three Seyfert Galaxies

2003 ◽  
Vol 126 (1) ◽  
pp. 143-152 ◽  
Author(s):  
B. T. Soifer ◽  
J. J. Bock ◽  
K. Marsh ◽  
G. Neugebauer ◽  
K. Matthews ◽  
...  
Keyword(s):  
Spatial Resolution ◽  
High Spatial Resolution ◽  
Seyfert Galaxies ◽  
Mid Infrared ◽  
Infrared Observations
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