The central region of NGC 1510

B, V, and R plates of the central portion of NGC 1510 show a complex structure of several condensations which exhibit different colors. Blue and red spectra of two of these condensations indicate that they are low density and slightly metal-poor H II regions with an underlying A-star component. The...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 1984-03, Vol.132 (2), p.342-350
Hauptverfasser: EICHENDORF, W, NIETO, J.-L
Format: Artikel
Sprache:eng
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Zusammenfassung:B, V, and R plates of the central portion of NGC 1510 show a complex structure of several condensations which exhibit different colors. Blue and red spectra of two of these condensations indicate that they are low density and slightly metal-poor H II regions with an underlying A-star component. The mot convincing interperation of these observations appears to be that of an amorphous galaxy which accretes H I from the large halo of NGC 1512.
ISSN:0004-6361
1432-0746