LAMOST Medium-Resolution Spectral Survey of Galactic Nebula (LAMOST MRS-N): An overview of Scientific goals and Survey plan. (arXiv:2007.05240v1 [astro-ph.GA])
<a href="http://arxiv.org/find/astro-ph/1/au:+Wu_C/0/1/0/all/0/1">Chao-Jian Wu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wu_H/0/1/0/all/0/1">Hong Wu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_W/0/1/0/all/0/1">Wei Zhang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ren_J/0/1/0/all/0/1">Juan-Juan Ren</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chen_J/0/1/0/all/0/1">Jian-Jun Chen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hsia_C/0/1/0/all/0/1">Chih-Hao Hsia</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wu_Y/0/1/0/all/0/1">Yu-Zhong Wu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhu_H/0/1/0/all/0/1">Hui Zhu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Li_B/0/1/0/all/0/1">Bin Li</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hou_Y/0/1/0/all/0/1">Yong-Hui Hou</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wang_J/0/1/0/all/0/1">Jun-Lin Wang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yu_S/0/1/0/all/0/1">Shuo-Ran Yu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Collaboration_LAMOST_MRS/0/1/0/all/0/1">LAMOST MRS Collaboration</a>

Since Sep. 2018, LAMOST started the medium-resolution (R $sim 7500$)
spectral survey (MRS). We proposed the spectral survey of Galactic nebulae,
including hii regions, HH objects, supernova remnants, planetary nebulae and
the special stars with MRS (LAMOST MRS-N). LAMOST MRS-N covers about 1700
square degrees of the northern Galactic plane within $40^circ < l < 215^circ$
and $-5^circ < b < 5^circ$. In this 5-year survey, we plan to observe about
500 thousand nebulae spectra. According to the commissioning observations, the
nebulae spectra can provide precise radial velocity with uncertainty less than
1 km s$^{-1}$. These high-precision spectral data are of great significance to
our understanding of star formation and evolution.

Since Sep. 2018, LAMOST started the medium-resolution (R $sim 7500$)
spectral survey (MRS). We proposed the spectral survey of Galactic nebulae,
including hii regions, HH objects, supernova remnants, planetary nebulae and
the special stars with MRS (LAMOST MRS-N). LAMOST MRS-N covers about 1700
square degrees of the northern Galactic plane within $40^circ < l < 215^circ$
and $-5^circ < b < 5^circ$. In this 5-year survey, we plan to observe about
500 thousand nebulae spectra. According to the commissioning observations, the
nebulae spectra can provide precise radial velocity with uncertainty less than
1 km s$^{-1}$. These high-precision spectral data are of great significance to
our understanding of star formation and evolution.

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