IR light curves of four new low-mass eclipsing binaries
In the last decade a significant amount of observational effort has been made to determine the physical parameters of low mass stars (M 1 Msol). The most...
We report, as a part of a long-term study of IR mergers and IR QSOs, detailed spectroscopic evidences for outflow (OF) features in nearby IR mergers/QSOs (with...
IR photometry of Alpha Per low-mass members (Lodieu+, 2005)
Optical detections in five different fields of view (A, C, E, K, and L) are matched with the near-infrared detections described in this paper. The central...
The results of medium resolution (R=600) spectrophotometry of 15 bright carbon stars of class N, obtained in the range of lambda:1 to 4.2 microns, are presented...
Warm IRAC [3.6] and [4.5] photometry is critical for understanding the cold population of brown dwarfs now being found, objects which have more in common with...
IRAM 30-meter millimeter follow-up of deep OSIRIS-GTC optical surveys
It is broadly accepted that CO is a reliable tracer of H2 in massive IR (L IR ≳ 10 9 L ⊙) galaxies, and that there are clear correlations between L IR and L' CO...