- from
magnitude 5.48 to 5.53 over a
period of 1.12 days. In 1981,
Robert Shobbrook announced that HR 3462 is a
variable star
based on
observations made in...
- doi:10.1093/mnras/sty1912. Mkrtichian, D. E.; Hatzes, A. P.; Saio, H.;
Shobbrook, R. R. (2008). "The
detection of the rich p-mode
spectrum and asteroseismology...
- of
Stellar Radial Velocities", Washington, Bibcode:1953GCRV..C......0W
Shobbrook, R. R.; Handler, G.; Lorenz, D.; Mogorosi, D. (2006). "Photometric studies...
- 143018)", The Observatory, 116: 387–391, Bibcode:1996Obs...116..387S
Shobbrook, R. R. (December 2005), "Photometry of 20
eclipsing and
ellipsoidal binary...
- of
Variable Star Observers.
Retrieved 2
February 2014. Stobie, R. S.;
Shobbrook, R. R. (1976). "Frequency
Analysis of the
Delta Scuti star,
Theta Tucanae"...
- Light. The land west of
Goodwood Road was
purchased from the
Estate of
Shobbrooks, and a
smaller block was
purchased from A. Hann. This
became part of Colonel...
- Astronomy) 天文教育資訊網 2006 年 7 月 25 日
Archived 2011-05-22 at the
Wayback Machine Shobbrook, R. R. (1972). "Two new Beta
Canis Majoris variables:
epsilon Cen and...
- Nesvacil, N.; Hempel, A.; Romero-Colmenero, E.; Vuthela, F. F.; Reegen, P.;
Shobbrook, R. R.; Kilkenny, D. (30
August 2002). "On the Period-Luminosity-Colour-Metallicity...
-
American ****ociation of
Variable Star Observers.
Retrieved 18
February 2014.
Shobbrook, R. R. (December 2005). "Photometry of 20
eclipsing and
ellipsoidal binary...
-
rotational line
broadening was observed, by
Frank Schlesinger in 1911.
Shobbrook, R. R. (December 2005). "Photometry of 20
eclipsing and
ellipsoidal binary...
