搜索结果: 16-29 共查到“知识库 天文学 continuum”相关记录29条 . 查询时间(0.234 秒)
Accretion Disks and the Nature and Origin of AGN Continuum Variability
Accretion Disks AGN Continuum Variability
2009/7/9
Accretion Disks and the Nature and Origin of AGN Continuum Variability。
Radio continuum sources associated with AB Aur。
Radio Continuum and H92 Recombination Line Observations of G34.26+0.15 and G5.89-0.39
G34.26+0.15 G5.89-0.39 H92 Recombination Line
2009/6/11
Radio Continuum and H92 Recombination Line Observations of G34.26+0.15 and G5.89-0.39。
Radio Continuum Observations towards Optical and Molecular Outflows
Optical Molecular Outflows
2009/6/11
Radio Continuum Observations towards Optical and Molecular Outflows。
Time Variation in the Radio Continuum Emission Associated with the Surroundings of the Nucleus of the Planetary Nebula KjPn 8
Radio Continuum Emission KjPn 8 Planetary Nebula
2009/6/11
Time Variation in the Radio Continuum Emission Associated with the Surroundings of the Nucleus of the Planetary Nebula KjPn 8。
Radio continuum and h i observations of the remarkable planetary nebula KJPN 8
h i observations KJPN 8 remarkable planetary nebula
2009/6/11
Radio continuum and h i observations of the remarkable planetary nebula KJPN 8
VLA radio continuum observations of WR ring nebulae。
Ionizing Continuum and Emission-Line Energetics of Quasars and Seyfert Galaxies
Quasars Seyfert Galaxies Ionizing Continuum
2009/6/9
Ionizing Continuum and Emission-Line Energetics of Quasars and Seyfert Galaxies。
The puzzle of the lyman continuum polarization of qsos
lyman continuum polarization of qsos
2009/6/8
The puzzle of the lyman continuum polarization of qsos。
Radio Continuum and H I Observations of the Remarkable Planetary Nebula KJPN 8
Radio Continuum Planetary Nebulae
2009/6/4
Radio Continuum and H I Observations of the Remarkable Planetary Nebula KJPN 8
Radio Continuum and Far-infrared Emission from the Galaxies in the Eridanus Group
radio continuum radio–FIR correlation galaxies
2009/5/12
The Eridanus galaxies follow the well-known radio–FIR
correlation. The majority (70%) of these galaxies have their star formation
rates below that of the Milky Way. The galaxies that have a signific...
A RADIO-CONTINUUM STUDY OF THE SUPERNOVA REMNANT MSH 11-61A
ISM individual objects (MSH 11-61A, G290.1-0.8)-ISM supernova remnants-radio continuum ISM
2009/2/26
We present a high-resolution radio-continuum study of Galactic
supernova remnant MSH11{61A. We combine moderate resolution X-ray, radio-
continuum and CO data to study the morphology and kinematics ...
RADIO CONTINUUM STUDY OF THE LARGE MAGELLANIC CLOUD - SNR J0519-6926
ISM supernova remnants-Magellanic Clouds-ISM individual ob-jects SNR J0519-6926
2009/2/9
We present the results of new high resolution ATCA observations
of SNR J0519{6926. We found that this SNR exhibits a typical "horseshoe" ap-
pearance with ®={0.55§0.08 and D=28§1 pc. No polariza...
RADIO-CONTINUUM STUDY OF THE SUPERNOVA REMNANTS IN THE LARGE MAGELLANIC CLOUD-AN SNR WITH A HIGHLY POLARISED BREAKOUT REGION-SNR J0455-6838
ISM supernova remnants-Magellanic Clouds-Radio Continuum ISM-Polarization-ISM individual objects-SNR J0455-6838
2009/1/19
We present the results of new moderate resolution ATCA obser-
vations of SNR J0455{6838. We found that this SNR exhibits a mostly typical
appearance with rather steep and curved ®={0.81§0.18 and...