The H/r Diagram of NGC1962 NGC1965 NGC1966 NGC1970

Details The H/r Diagram of NGC1962 NGC1965 NGC1966 NGC1970 The H/r Diagram of NGC1962 NGC1965 NGC1966 NGC1970

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108...35s&link_type=abstract

Structure and Evolution of the Magellanic Clouds, Proceedings of IAU Symposium No. 108, held 5-8 September 1983 in Tübingen, Wes

Computer Science

3

Scientific paper

The complex NGC 1962-65-66-70 is one of the many giant filamentary shell
nebulae in the LMC. The nebulosity surrounds an association of very
young blue stars. The authors have obtained UBV photometry and IUE
spectra of the bright members of the association and have used these
data to construct the H-R diagram and to derive ages for these stars.

Affiliated with

Also associated with

No associations

Rating

The H/r Diagram of NGC1962 NGC1965 NGC1966 NGC1970 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The H/r Diagram of NGC1962 NGC1965 NGC1966 NGC1970, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The H/r Diagram of NGC1962 NGC1965 NGC1966 NGC1970 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1395149