The interstellar extinction law towards the open cluster TR-37

Details The interstellar extinction law towards the open cluster TR-37 The interstellar extinction law towards the open cluster TR-37

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.233..773r&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 233, Aug. 15, 1988, p. 773-779.

Astronomy and Astrophysics

Astronomy

14

H Ii Regions, Infrared Photometry, Interstellar Extinction, Open Clusters, Stellar Mass, Ultraviolet Astronomy, Far Ultraviolet Radiation, Near Infrared Radiation

Scientific paper

Near-infrared photometry of OB stars in the young open cluster TR-37 has been obtained. These data have been combined with previous visual and ultraviolet observations of the same sample and a detailed extinction curve has been derived, ranging from the near-infrared to the far-ultraviolet. The extinction towards this sample of stars seems to be anomalous, consistent with a shift in the grain-size distribution with respect to an average galactic extinction curve.

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