搜索结果: 1-9 共查到“星系与宇宙学 magellanic cloud”相关记录9条 . 查询时间(0.05 秒)
A combination of analytic models and n-body simulations implies that the structural evolution of the Large Magellanic Cloud (LMC) is dominated by its dynamical interaction with the Milky Way. Although...
X-RAY AND ULTRAVIOLET SPECTROSCOPY OF GALACTIC DIFFUSE HOT GAS ALONG THE LARGE MAGELLANIC CLOUD X-3 SIGHT LINE
diffuse background halo
2014/12/23
We present Suzaku spectra of X-ray emission in the fields just off the LMC X-3 sight line. O VII, O VIII, and Ne IX emission lines are clearly detected, suggesting the presence of an optically thin th...
Variable Stars in Large Magellanic Cloud Globular Clusters I: NGC 1466
Variable Stars Large Magellanic Cloud Globular Clusters
2011/10/18
This is the first in a series of papers studying the variable stars in Large Magellanic Cloud globular clusters. The primary goal of this series is to better understand how the RR Lyrae stars in Ooste...
The proper motion of the large magellanic cloud：a reanalysis
proper motion magellanic cloud
2009/6/25
The proper motion of the large magellanic cloud：a reanalysis。
Light echoes of supernovae in the large magellanic cloud
supernovae large magellanic cloud
2009/6/25
Light echoes of supernovae in the large magellanic cloud。
Hot gas in the large magellanic cloud。
THE RELATION BETWEEN RADIO FLUX DENSITY AND IONISING ULTRA-VIOLET FLUX FOR HII REGIONS AND SUPERNOVA REMNANTS IN THE LARGE MAGELLANIC CLOUD
Galaxies Magellanic Clouds-ISM HII regions-ISM supernova remnants-radio continuum galaxies-ultraviolet galaxies
2009/3/12
We present a comparison between the Parkes radio surveys (Filipovi
´c et al. 1995) and Vacuum Ultra-Violet (VUV) surveys (Smith et al. 1987)
of the Large Magellanic Clouds (LMC). We have found...
THE STRONGEST 100 RADIO POINT SOURCES IN THE FIELD OF THE LARGE MAGELLANIC CLOUD AT 1.4 GHz
Radio Continuum: galaxies Magellanic Clouds Catalogs
2010/10/29
We present the 100 strongest 1.4 GHz point sources from a new mosaic image in the direction of the Large Magellanic Cloud (LMC). The observations making up the mosaic were made using Australia Telesco...
OPTICAL SPECTRA OF RADIO PLANETARY NEBULAE IN THE LARGE MAGELLANIC CLOUD
planetary nebulae individual SMP L8 SMP L25 SMP L33 SMP L39 SMP L47 SMP L62 SMP L74 SMP L75 SMP L83 SMP L84 SMP L89
2009/1/16
We present 11 spectra from 12 candidate radio sources co-identi¯ed
with known planetary nebulae (PNe) in the Large Magellanic Cloud (LMC). Origi-
nally found in Australia Telescope Compact Arra...