On the radial oxygen distribution in the Galactic disc - II. Effects of local streams

被引:1
作者
Mishurov, Yu. N. [1 ]
Tkachenko, R. V. [1 ]
机构
[1] Southern Fed Univ, Fac Phys, 5 Zorge, Rostov Na Donu 344090, Russia
关键词
Galaxy: abundances; Galaxy: disc; Galaxy: evolution; MILKY-WAY; GAS;
D O I
10.1093/mnras/sty628
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We analyse the idea that the local dips (similar to 1 kpc along the Galactic radius) observed in oxygen abundance are associated with the infall of intergalactic low-abundant gas (similar to 0.2 Z(circle dot)) on to the Galactic disc during the last similar to 100 Myr. We term such infall events local streams. The derived masses of the falling gas (of the order of several times 10(8) M-circle dot) are close to the observed ones (e.g. in the Magellanic Stream). Such local streams do not change the mean mass of oxygen ejected per core-collapse supernova (CC SN) event, so that our previous inference on probable upper initial masses for progenitors of CC SNe remains valid.
引用
收藏
页码:5377 / 5381
页数:5
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