North-PHASE: Studying periodicity, hot spots, accretion stability, and early evolution in young stars in the Northern hemisphere

Sicilia-Aguilar A.; Kahar R.S.; Pelayo-Baldárrago M.E.; Roccatagliata V.; Froebrich D.; Galindo-Guil F.J.; Campbell-White J.; Kim J.S.; Mendigutía I.; Schlueter L.; Teixeira P.S.; Matsumura S.; Fang M.; Scholz A.; Ábrahám P.; Frasca A.; Garufi A.; Herbert C.; Kóspál Á.; Manara C.F. · Monthly Notices of the Royal Astronomical Society (2024) · DOI: 10.1093/mnras/stae1588

Resumen

We present the overview and first results from the North-PHASE Legacy Survey, which follows six young clusters for five years, using the 2 deg FoV of the JAST80 telescope from the Javalambre Observatory (Spain). North-PHASE investigates stellar variability on time-scales from days to years for thousands of young stars distributed over entire clusters. This allows us to find new YSO, characterize accretion, and study inner disc evolution within the cluster context. Each region (Tr 37, Cep OB3, IC 5070, IC 348, NGC 2264, and NGC 1333) is observed in six filters (SDSS griz, u band, and J0660, which covers H), detecting cluster members as well as field variable stars. Tr 37 is used to prove feasibility and optimize the variability analysis techniques. In Tr 37, variability reveals 50 new YSO, most of them proper motion outliers. North-PHASE independently confirms the youth of astrometric members, efficiently distinguishes accreting and non-accreting stars, reveals the extent of the cluster populations along Tr37/IC 1396 bright rims, and detects variability resulting from rotation, dips, and irregular bursts. The proper motion outliers unveil a more complex star formation history than inferred from Gaia alone, and variability highlights previously hidden proper motion deviations in the surrounding clouds. We also find that non-YSO variables identified by North-PHASE cover a different variability parameter space and include long-period variables, eclipsing binaries, RR Lyr, and Scuti stars. These early results also emphasize the power of variability to complete the picture of star formation where it is missed by astrometry.

Instituciones: Universidad Nacional Mayor de San Marcos