IR photometry around IRAS 16571-4029 (Roman-Lopes+, 2007)

Details IR photometry around IRAS 16571-4029 (Roman-Lopes+, 2007) IR photometry around IRAS 16571-4029 (Roman-Lopes+, 2007)

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..34710813r&link_type=abstract

VizieR On-line Data Catalog: J/A+A/471/813. Originally published in: 2007A&A...471..813R

Astronomy and Astrophysics

Astronomy

Stars: Pre-Main Sequence, Infrared Sources, Photometry: Infrared

Scientific paper

The stellar population was studied by using color-color and color-magnitude diagrams, as well as by analysing the spectral energy distributions in the near- and mid-infrared wavelengths. The extended emission was studied by the construction of contour diagrams, which were compared with near- and mid-infrared images. We computed the corresponding number of Lyman continuum photons (using the integrated Br{gamma} flux density) and compared it with that obtained from the 5GHz flux density to derive a mean visual extinction.
The NIR images were taken in the 2004 May observing run, using the Near Infrared Camera (CamIV) of the Laboratorio Nacional de Astrofisica, Brazil, which is based on a Hawaii 1024x1024 HgCdTe detector, attached to the 1.6m Perkin-Elmer telescope.
(1 data file).

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