Identification and NIR photometry of the Arecibo sample of OH/IR stars

Details Identification and NIR photometry of the Arecibo sample of OH/IR stars Identification and NIR photometry of the Arecibo sample of OH/IR stars

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..223j&link_type=abstract

In: Mass-losing pulsating stars and their circumstellar matter. Workshop, May 13-16, 2002, Sendai, Japan, edited by Y. Nakada, M

Astronomy and Astrophysics

Astrophysics

Oh/Ir Stars, Near-Infrared

Scientific paper

In June 1999 we started a near-infrared (NIR) monitoring of the full Arecibo sample of OH/IR stars (385 sources) using the 1.23 m telescope at Calar Alto Observatory equipped with the MAGIC IR camera. Since then, we have completed 6 observing runs and obtained J, H and K images of almost all sources in the sample (97%) under good photometric conditions. NIR and optical counterparts have been identified and NIR photometric data has also been obtained.

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