Cepheids in the young LMC cluster NGC 1866 (Storm+, 2005)

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Magellanic Clouds, Clusters: Globular, Stars: Variable, Photometry: Infrared, Radial Velocities

Scientific paper

Near-infrared photometric light (K-band) and color (J-K) curves are presented for six Cepheids the Large Magellanic Cloud cluster NGC 1866 in Table 1. Barycentric velocity curves for these stars as well as for four additional cluster Cepheids and two Cepheids in the LMC cluster NGC 2031 are presented in Table 2. The systemic (gamma) velocities for these stars are presented in table 4.
(3 data files).

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Cepheids in the young LMC cluster NGC 1866 (Storm+, 2005) 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 Cepheids in the young LMC cluster NGC 1866 (Storm+, 2005), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cepheids in the young LMC cluster NGC 1866 (Storm+, 2005) will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1168281

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.