CCD Photometry of the δ Scuti star FG Virginis During the 1995 Multi-Site Campaign

Details CCD Photometry of the δ Scuti star FG Virginis During the 1995 Multi-Site Campaign CCD Photometry of the δ Scuti star FG Virginis During the 1995 Multi-Site Campaign

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.260..281s&link_type=abstract

Astrophysics and Space Science, v. 260, Issue 3, p. 281-290 (1999).

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

The results of the CCD photometry of the 1995 FG Virginis multi-site campaign, organized by the Delta Scuti Network, are presented. Between March 16 and April 20, 1995 over 120 hours of CCD measurements were obtained. The ten frequencies of FG Vir, known from the previous campaign (1993), range from 9.20 to 34.12 cycles/day (106.5 and 394.9 μHz). Three new frequencies at 16.07, 19.23 and 24.19 c/d (186.0, 222.5 and 279.9 μHz) were detected. The precision of the FG Vir measurements was better than 3.5 mmag per single 1-min integration. It is shown that the present CCD measurements are of similar quality as those obtained simultaneously by photometers with photomultiplier detectors using the three-star observing technique.

Affiliated with

Also associated with

No associations

Rating

CCD Photometry of the δ Scuti star FG Virginis During the 1995 Multi-Site Campaign 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 CCD Photometry of the δ Scuti star FG Virginis During the 1995 Multi-Site Campaign, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CCD Photometry of the δ Scuti star FG Virginis During the 1995 Multi-Site Campaign will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1074608