The stars and gas in the region of N63A (LMC)

Details The stars and gas in the region of N63A (LMC) The stars and gas in the region of N63A (LMC)

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...164...26l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 164, no. 1, Aug. 1986, p. 26-30.

Astronomy and Astrophysics

Astrophysics

7

Interstellar Gas, Magellanic Clouds, Star Clusters, Supernova Remnants, Astronomical Photometry, Gas Dynamics, H Alpha Line, Hertzsprung-Russell Diagram, Hydrogen Clouds, Stellar Color

Scientific paper

N 63A is located in the cluster NGC 2030 of the LMC. From VBLUW observations of some cluster stars the authors derive AV = 0.6 mag reddening in the direction of N 63A; the age of the cluster is estimated as ≡4×106yr. VBLUW observations indicate the western knot of N 63A to be excited by an 05-9 main sequence star. The north-eastern and southern knots form the known SNR. Fabry-Perot observations indicate a velocity range of 100 - 300 km s-1 for the SNR gas.

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