In this paper, we consider the full compressible Navier–Stokes equations in d="mmlsi1" class="mathmlsrc">data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S146812181630058X&_mathId=si1.gif&_user=111111111&_pii=S146812181630058X&_rdoc=1&_issn=14681218&md5=a568fb5d436c2a74eaf4727f0c70f51f" title="Click to view the MathML source">Ndden">de">(d="mmlsi2" class="mathmlsrc">data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S146812181630058X&_mathId=si2.gif&_user=111111111&_pii=S146812181630058X&_rdoc=1&_issn=14681218&md5=970e91f3784e66cf32d86795abc4bcd7" title="Click to view the MathML source">N≥2dden">de">) space dimension with cylindrical or spherical symmetric initial data. The global existence of strong and classical solutions is established. The analysis is based on some delicate a priori estimates which depend on the assumption d="mmlsi3" class="mathmlsrc">data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S146812181630058X&_mathId=si3.gif&_user=111111111&_pii=S146812181630058X&_rdoc=1&_issn=14681218&md5=01f434e8d3cbe706844dbeb820ba6bef" title="Click to view the MathML source">κ(θ)=θqdden">de"> where d="mmlsi4" class="mathmlsrc">data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S146812181630058X&_mathId=si4.gif&_user=111111111&_pii=S146812181630058X&_rdoc=1&_issn=14681218&md5=2c63c36eff4d2a99c761cdc898dead2b" title="Click to view the MathML source">q⩾0dden">de"> and d="mmlsi5" class="mathmlsrc">data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S146812181630058X&_mathId=si5.gif&_user=111111111&_pii=S146812181630058X&_rdoc=1&_issn=14681218&md5=e4afc4c1831ca38dbd8e37c3bcea0cbf">dth="223" alt="View the MathML source" title="View the MathML source" src="/sd/grey_pxl.gif" data-inlimgeid="1-s2.0-S146812181630058X-si5.gif">dden">de">. Compared with the results in Wen and Zhu (2014) and Qin, Yang, Yao and Zhou (2015), our results relax the restriction d="mmlsi6" class="mathmlsrc">data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S146812181630058X&_mathId=si6.gif&_user=111111111&_pii=S146812181630058X&_rdoc=1&_issn=14681218&md5=67b6ebe6f685a82b3858edfb75928ab2" title="Click to view the MathML source">q>0dden">de">, when there is no initial vacuum and include the global existence of classical solutions for both the cylindrical or spherical symmetric cases, respectively. It should point out that we obtain the global classical solutions with the help of weighted d="mmlsi7" class="mathmlsrc">data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S146812181630058X&_mathId=si7.gif&_user=111111111&_pii=S146812181630058X&_rdoc=1&_issn=14681218&md5=16a1a23c0125549034791b5657984edf" title="Click to view the MathML source">H3dden">de"> estimates of d="mmlsi8" class="mathmlsrc">data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S146812181630058X&_mathId=si8.gif&_user=111111111&_pii=S146812181630058X&_rdoc=1&_issn=14681218&md5=99930ba861687a9c10381aff51089309" title="Click to view the MathML source">(u,v,w,θ)dden">de">.