A Spectroscopic and Photometric Study of Young Embedded Stars in NGC 2024

Details A Spectroscopic and Photometric Study of Young Embedded Stars in NGC 2024 A Spectroscopic and Photometric Study of Young Embedded Stars in NGC 2024

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aas...187.6602a&link_type=abstract

American Astronomical Society, 187th AAS Meeting, #66.02; Bulletin of the American Astronomical Society, Vol. 27, p.1376

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We present estimates for the effective temperature, luminosity, extinction and excess infrared emission for ~ 40 members of the young embedded cluster NGC 2024. These results were derived from infrared (2.15-2.35 mu m) spectroscopy and J, H, K and L(') \ photometry. We estimate the masses and ages of these stars by comparing their location on the H-R diagram to theoretical pre-main sequence evolutionary tracks. These results are used to explore issues of co-evality, mass and/or age segregation and disk activity in NGC 2024.

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