搜索结果: 1-15 共查到“理学 Large Magellanic Cloud”相关记录15条 . 查询时间(0.14 秒)
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 Global Gas and Dust budge of the Large Magellanic Cloud --- Importance of Asymptotic Giant Branch stars
The Global Gas Large Magellanic Cloud
2010/11/11
It is still an unresolved problemhowmuch AGB stars can contribute to the overall gas and dust enrichment processes in the interstellar medium within galaxies.We start tackling this problem, by using o...
Dust at sub-solar metallicity: the case of post-AGB stars in the Large Magellanic Cloud
Dust at sub-solar metallicity Large Magellanic Cloud
2010/11/11
Low- and intermediate-mass stars are one of the important dust sources in the interstellar medium (ISM) of galaxies. The compositions of dust ejected from these stars are likely to affect those in the...
The star formation history of the Large Magellanic Cloud as seen by star clusters and stars
galaxies evolution - galaxies: individual galaxies stellar content - galaxies star clusters
2010/11/10
The aim of this work is to test to what extent the star cluster population of a galaxy can be
utilised to constrain or estimate the star formation history, with the Large Magellanic Cloud as our test...
Survey of O VI absorption in the Large Magellanic Cloud
galaxies ISM – ISM structure – ISM atoms – galaxies individual Large Magellanic Cloud – ultraviolet ISM
2010/11/10
We present a survey of interstellar O VI absorption in the Large Magellanic Cloud (LMC) towards 70 lines of sight based on Far Ultraviolet Spectroscopic Explorer(FUSE) observations. The survey covers ...
Assessment of Stellar Stratification in Three Young Star Clusters in the Large Magellanic Cloud
Magellanic Clouds galaxies star clusters globular clusters individual NGC 1983,NGC 2002, NGC 2010 Hertzsprung-Russell diagram Methods statistical stellar dynamics
2010/3/8
(abridged) We present a comprehensive study of stellar stratification in young star clusters in the Large Magellanic Cloud (LMC). We apply our recently developed effective radius method for the assess...
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...
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...
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...
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...
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...