[CGC2008] N180 27C , the SIMBAD biblio

We used Spitzer infrared observations to find the young stars of two H II regions in the Large Magellanic Cloud, N63 and N180. The young stellar object (YSO) candidates were identified in each nebula by means of color-color, color-magnitude diagrams, and the shapes of their spectral energy distributions (SEDs). The most luminous YSOs are found near the ionization fronts within strong 8 µm emission clumps. Most YSOs, less luminous, are seen in projection inside the H II regions. HST images show several Class I stars that have emerged along the borders of the H II regions; other YSOs are embedded in cometary clouds. The most luminous YSO of N63 is connected to a string of pointlike sources. Its SED can be modeled by a central source of stellar mass M_* between 7 and 11 M_☉, with a circumstellar disk of outer radius R_d of ∼55 AU, and an envelope of moderate accretion rate, M{dot}_env of ∼2x10^–5 M_☉/yr. N180 is experiencing a phase of star formation more intense than N63, attested by the properties of its most luminous YSO: M_* of 25 M_☉, R_dof ∼200 AU, and M{dot}_envof ∼1.5x10^–3 M_☉/yr. The modes of triggered star formation in N63 and N180 appear similar to those seen in Galactic H II regions.