BVRI photometry of the extrinsic S star HR 1105

Details BVRI photometry of the extrinsic S star HR 1105 BVRI photometry of the extrinsic S star HR 1105

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...333..952a&link_type=abstract

Astronomy and Astrophysics, v.333, p.952-955 (1998)

Other

1

Stars: Agb, Post Agb, Binaries: Close, Stars:Individual: Hr 1105, Stars: Variables: Other

Scientific paper

BVRI photometry of the extrinsic S star HR 1105 shows a stable periodic light variability with a period of 24.76 days superimposed upon long term changes presumably related to the orbital period. The variations are in phase for all four magnitudes with the amplitude of this variability being about the same for B and V, but smaller for R and even smaller for I. As the primary is a M3 III star, these brightness changes are mostly likely due to the pulsation of the primary star. Table 1 is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html

Affiliated with

Also associated with

No associations

Rating

BVRI photometry of the extrinsic S star HR 1105 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 BVRI photometry of the extrinsic S star HR 1105, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and BVRI photometry of the extrinsic S star HR 1105 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1363187