Emission-Line Imaging of QSO[CLC]s[/CLC] with High Resolution

2001 ◽  
Vol 121 (1) ◽  
pp. 80-89 ◽  
Author(s):  
J. B. Hutchings ◽  
S. L. Morris ◽  
D. Crampton
Keyword(s):  
High Resolution ◽  
Emission Line ◽  
Line Imaging

scholarly journals High resolution spectroscopy and emission line imaging of DEM L 71 withXMM-Newton

2003 ◽  
Vol 406 (1) ◽  
pp. 141-148 ◽  
Author(s):  
K. J. van der Heyden ◽  
J. A. M. Bleeker ◽  
J. S. Kaastra ◽  
J. Vink
Keyword(s):  
High Resolution ◽  
Emission Line ◽  
High Resolution Spectroscopy ◽  
Line Imaging

FeXIV Line Emission Polarization of the July 11, 1991 Solar Corona

1994 ◽  
Vol 144 ◽  
pp. 541-547
Author(s):  
J. Sýkora ◽  
J. Rybák ◽  
P. Ambrož
Keyword(s):  
High Resolution ◽  
Solar Corona ◽  
Emission Line ◽  
Solar Eclipse ◽  
White Light ◽  
Preliminary Analysis ◽  
Line Emission ◽  
Total Solar Eclipse ◽  
Degree Of Polarization ◽  
High Resolution Images

AbstractHigh resolution images, obtained during July 11, 1991 total solar eclipse, allowed us to estimate the degree of solar corona polarization in the light of FeXIV 530.3 nm emission line and in the white light, as well. Very preliminary analysis reveals remarkable differences in the degree of polarization for both sets of data, particularly as for level of polarization and its distribution around the Sun’s limb.

scholarly journals High Resolution CO Imaging of a Cometary Globule in the Helix Nebula

2003 ◽  
Vol 209 ◽  
pp. 277-278
Author(s):  
P. J. Huggins ◽  
T. Forveille ◽  
R. Bachiller ◽  
P. Cox
Keyword(s):  
High Resolution ◽  
Neutral Gas ◽  
Line Imaging

We report high resolution CO (1–0) line imaging of a prominent cometary globule in the Helix Nebula. The results confirm earlier observations (Huggins et al. 1992) that globules consist of dense condensations of neutral gas embedded in the ionized nebula, and they provide new constraints on the structure and kinematics of the gas.

scholarly journals Tomography of AM Her and QQ Vul

2004 ◽  
Vol 190 ◽  
pp. 251-257 ◽  
Author(s):  
A. Staude ◽  
A. D. Schwope ◽  
P. Hedelt ◽  
A. Rau ◽  
R. Schwarz
Keyword(s):  
High Resolution ◽  
Emission Line ◽  
Imaging Techniques ◽  
High Resolution Spectroscopy

AbstractWe present optical high-resolution spectroscopy of AM Her and QQ Vul. Making use of indirect imaging techniques (Doppler and Roche tomography), we are able to make details visible, which a model of these systems has to be able to account for. Especially the emission line data cannot be explained by current models of polars.

A high-resolution Fabry-P�rot spectrometer for emission line studies in planetary nebulae and other extended astronomical objects

1987 ◽  
Vol 139 (2) ◽  
pp. 327-335
Author(s):  
D. P. K. Banerjee ◽  
B. G. Anandarao ◽  
J. N. Desai ◽  
N. S. Jog ◽  
P. K. Kikani ◽  
...  
Keyword(s):  
High Resolution ◽  
Emission Line ◽  
Planetary Nebulae

An Emission-Line Imaging Survey of Early-Type Seyfert Galaxies. II. Implications for Unified Schemes

1996 ◽  
Vol 467 ◽  
pp. 197 ◽  
Author(s):  
John S. Mulchaey ◽  
Andrew S. Wilson ◽  
Zlatan Tsvetanov
Keyword(s):  
Emission Line ◽  
Seyfert Galaxies ◽  
Early Type ◽  
Line Imaging

Emission-Line Imaging of 3CR Radio Galaxies. I. Imaging Data

1995 ◽  
Vol 99 ◽  
pp. 27 ◽  
Author(s):  
Patrick J. McCarthy ◽  
Hyron Spinrad ◽  
Wil van Breugel
Keyword(s):  
Emission Line ◽  
Radio Galaxies ◽  
Imaging Data ◽  
Line Imaging

scholarly journals Near-IR emission line imaging of PN

1997 ◽  
Vol 180 ◽  
pp. 237-237
Author(s):  
T.M. Hodge ◽  
C.E. Woodward ◽  
D.M. Kelly ◽  
J. Fischer ◽  
M. A. Greenhouse ◽  
...  
Keyword(s):  
Emission Line ◽  
Ionization Potential ◽  
Orion Nebula ◽  
Spatial Studies ◽  
Spatially Resolved ◽  
Ngc 7027 ◽  
Line Imaging ◽  
Ngc 7662 ◽  
Physical And Chemical ◽  
Ir Emission

Spatial studies of the emission line regions in planetary nebulae (PN) can provide insight into the physical and chemical environments across the nebulae. In a collaborative effort by the coauthors, a K-band Fabry-Perot etalon has been coupled with an advanced 256 × 256 InSb focal plane array at the Wyoming Infrared Observatory 2.3m telescope. This system permits us to obtain spatially resolved, 0.24″/pixel, moderate spectral resolution (R ≈ 800), flux-density IR emission line images of astronomical sources. We obtained continuum-subtracted images of Br γ, HeI 2.06 μm, the 2-μm UIR features, and the 3.3 μm PAH dust feature in the PN NGC 6572, NGC 7027, and NGC 7662. One objective was to determine the spatial morphology of two unidentified emission lines, UIR1−2.199 μm, and UIR2−2.287 μm (Geballe et al. 1991). These UIR lines appear in the spectra of many PN (Hora et al. 1997) and in the Orion Nebula (Luhman & Rieke 1996). Geballe et al. suggested that the UIR lines are most likely forbidden transitions and showed that the parent ion ionization potential is ≈ 30–40 eV, while the ionization potential for the ions themselves is 40–60 eV. Here we directly compare the distribution of the UIR emitters to that of the gas (H+,He+) and dust (PAHs).

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