International audienceAims. We identify the stellar populations (mostly red giants and young stars) detected in the ISOGAL survey at 7 and 15 μm towards a field (LN45) in the direction , .Methods. The sources detected in the survey of the Galactic plane by the Infrared Space Observatory were characterised based on colour-colour and colour-magnitude diagrams. We combine the ISOGAL catalogue with the data from surveys such as 2MASS and GLIMPSE. Interstellar extinction and distance were estimated using the red clump stars detected by 2MASS in combination with the isochrones for the AGB/RGB branch. Absolute magnitudes were thus derived and the stellar populations identified from their absolute magnitudes and their infrared excess.Results. A sta...
We present near-IR spectra (HK-band) of a sample of 107 sources with mid-IR excesses at 7 and 15$\;\...
In this work we present near-IR spectra (HK-band) of a sample of 107 sources with mid-IR excesses at...
Context: The stellar populations in the central region of the Galaxy are poorly known because of the...
International audienceAims. We identify the stellar populations (mostly red giants and young stars) ...
15 pages, 9 figures, accepted for publication in Astronomy and Astrophysics JournalThe ISOGAL projec...
We present and analyse the data of a field at 1 = 0°, b = +1° from the ISOGAL survey of se...
A&A in press. 19 pages,10 Ps figures; problems with figures fixedThe ISOGAL project is an infrared s...
ISOGAL is a survey at 7 and 15 μm with ISOCAM of the inner galactic disk and bulge of our Galaxy. Th...
International audienceISOGAL is a survey at 7 and 15 μm with ISOCAM of the inner galactic disk and b...
We report the study of ISOGAL fields in the outer galactic bulge. We have combined 7 and 15 μm ISOCA...
International audienceWe report the study of ISOGAL fields in the outer galactic bulge. We have comb...
16 pages, accepted for publication in Astronomy and AstrophysicsWe present a study of ISOGAL sources...
We report the study of ISOGAL fields in the outer galactic bulge. We have combined 7 and 15 μm ISOC...
ISOGAL, one of the most important programs observed by ISO, is a 7-15 μm ISOCAM survey, with 6" pixe...
The DENIS/ISOGAL near/mid-IR survey of the Milky Way for the first time probes stellar populations i...
We present near-IR spectra (HK-band) of a sample of 107 sources with mid-IR excesses at 7 and 15$\;\...
In this work we present near-IR spectra (HK-band) of a sample of 107 sources with mid-IR excesses at...
Context: The stellar populations in the central region of the Galaxy are poorly known because of the...
International audienceAims. We identify the stellar populations (mostly red giants and young stars) ...
15 pages, 9 figures, accepted for publication in Astronomy and Astrophysics JournalThe ISOGAL projec...
We present and analyse the data of a field at 1 = 0°, b = +1° from the ISOGAL survey of se...
A&A in press. 19 pages,10 Ps figures; problems with figures fixedThe ISOGAL project is an infrared s...
ISOGAL is a survey at 7 and 15 μm with ISOCAM of the inner galactic disk and bulge of our Galaxy. Th...
International audienceISOGAL is a survey at 7 and 15 μm with ISOCAM of the inner galactic disk and b...
We report the study of ISOGAL fields in the outer galactic bulge. We have combined 7 and 15 μm ISOCA...
International audienceWe report the study of ISOGAL fields in the outer galactic bulge. We have comb...
16 pages, accepted for publication in Astronomy and AstrophysicsWe present a study of ISOGAL sources...
We report the study of ISOGAL fields in the outer galactic bulge. We have combined 7 and 15 μm ISOC...
ISOGAL, one of the most important programs observed by ISO, is a 7-15 μm ISOCAM survey, with 6" pixe...
The DENIS/ISOGAL near/mid-IR survey of the Milky Way for the first time probes stellar populations i...
We present near-IR spectra (HK-band) of a sample of 107 sources with mid-IR excesses at 7 and 15$\;\...
In this work we present near-IR spectra (HK-band) of a sample of 107 sources with mid-IR excesses at...
Context: The stellar populations in the central region of the Galaxy are poorly known because of the...