Fig. 6.From: Infrared composition of the Large Magellanic CloudPosition of different types of objects in the color-magnitude diagrams N3–L24 vs. N3 (upper), N3–L24 vs. S7 (middle), S11–L24 vs. L24 (lower). (d) AGB candidates are shown as plus signs, (a) post-AGB stars as gray asterisks, (b) Mira stars as gray open triangles, (c) carbon stars as black filled triangles, (e) variable stars as X signs, (f) SRVs as gray open squares, and (g) OSARGs as diamonds.Back to article page