EUV mapping of the local interstellar medium: the Local Chimney revealed?
EUV mapping of the local interstellar medium: the Local Chimney revealed?
复制标题
当地星际介质的 EUV 测绘:当地烟囱显露出来?
DOI:
--
复制
发表时间:
1999
期刊:
影响因子:
--
通讯作者:
R. Lallement
中科院分区:
文献类型:
--
作者:
B. Welsh;D. Sfeir;M. Sirk;R. Lallement
We discuss the galactic distribution of 450 sources detected by the EUVE satellite that have reliable distance es- timates. Late-type stars dominate the nearby EUV source dis- tribution, whereas the majority of EUV source detections with distances > 100pc are hot white dwarf stars. The galactic dis- tribution of all these sources is non-uniform with number en- hancements seen towards the Hyades cluster, in line-of-sight along theCMa interstellar tunnel and towards high galactic latitudes in both hemispheres. A comparison of the distribution of these EUV sources with that of the neutral absorption bound- ary of the Local Bubble region derived from the interstellar NaI observations of Sfeir et al. (1999) reveals that vast majority of EUV sources are contained within this neutral boundary. How- ever, at high galactic latitudes 20 extragalactic EUV sources have been detected along lines-of-sight with low neutral column density, and is consistent with the local interstellar cavity being "open-ended" in the galactic halo. This "Local Chimney" opens towards two regions of enhanced intensity of the 0.25 keV soft X-ray background emission at high galactic latitudes. Although the hot Local Bubble gas is still contained within a cold, neutral interstellar gas boundary in the galactic plane, it has probably expanded into the halo to produce the Local Chimney feature.