Photometric confirmation of the δ Scuti pulsational variability in the pre-main-sequence Herbig Ae star HD104237

Details Photometric confirmation of the δ Scuti pulsational variability in the pre-main-sequence Herbig Ae star HD104237 Photometric confirmation of the δ Scuti pulsational variability in the pre-main-sequence Herbig Ae star HD104237

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999mnras.310.1071k&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 310, Issue 4, pp. 1071-1076.

Astronomy and Astrophysics

Astronomy

23

Stars: Emission-Line, Be, Stars: Individual: Hd104237, Stars: Oscillations, Stars: Pre-Main-Sequence, Δscuti

Scientific paper

Photometric observations of the Herbig Ae star HD104237 confirm that it is a δ Scuti star. We find two periods, the highest amplitude one having a value of 43min. This is only the fourth known pre-main-sequence δ Scuti star, and the only one with such short periods. These imply high-overtone modes which have not yet been investigated theoretically. Two of our comparison stars, HD104036 and 105234, are newly discovered δ Scuti stars.

Affiliated with

Also associated with

No associations

Rating

Photometric confirmation of the δ Scuti pulsational variability in the pre-main-sequence Herbig Ae star HD104237 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 Photometric confirmation of the δ Scuti pulsational variability in the pre-main-sequence Herbig Ae star HD104237, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photometric confirmation of the δ Scuti pulsational variability in the pre-main-sequence Herbig Ae star HD104237 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1580622