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Cited by 12 publications
(23 citation statements)
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“… References in Table 6: (1) Pribulla, Chochd & Parimueha (1999); (2) Gray et al (1996); (3) González et al (1996); (4) present paper (5) Qian & Liu (2000a); (6) Qian (2001); (7) Borkovits & Hegedues (1996); (8) Samec et al (1992); (9) Kim et al (1997); (10) Hobart, Pena & de La Cniz (1999); (11) Zhang et al (1989); (12) Liu & Yang (2000); (13) Derman & Demircan (1992); (14) Samec (1990); (15) Kaszás et al (1998); (16) Cerruti 1994; (17) Zhai, Leung & Zhang (1984); (18) Samec et al (1996); (19) Lipari & Sistero (1989); (20) Qian & Liu (2000b). …”
Section: Possible Relation Between the Period Change And The Mass Rmentioning
confidence: 99%
“… References in Table 6: (1) Pribulla, Chochd & Parimueha (1999); (2) Gray et al (1996); (3) González et al (1996); (4) present paper (5) Qian & Liu (2000a); (6) Qian (2001); (7) Borkovits & Hegedues (1996); (8) Samec et al (1992); (9) Kim et al (1997); (10) Hobart, Pena & de La Cniz (1999); (11) Zhang et al (1989); (12) Liu & Yang (2000); (13) Derman & Demircan (1992); (14) Samec (1990); (15) Kaszás et al (1998); (16) Cerruti 1994; (17) Zhai, Leung & Zhang (1984); (18) Samec et al (1996); (19) Lipari & Sistero (1989); (20) Qian & Liu (2000b). …”
Section: Possible Relation Between the Period Change And The Mass Rmentioning
confidence: 99%
“…For stars missing also from the list of Eggen the V -magnitudes from Hipparcos were taken. (1) Rucinski & Duerbeck (1997), (2) Maceroni & van't Veer (1996), (3) Eggen (1967), (4) Hipparcos catalogue, (5) Tycho catalogue, (6) Bradstreet (1985), (7) Samec et al (1989), (8) Samec (1990), (9) Samec et al (1991), (10) Samec et al (1993), (11) Broglia & Conconi (1983), (12) Zola et al (1997), (13) Hilditch et al (1989), (14) Stȩpień (1968), (15) Vinko et al (1996), (16) taken from Simbad or estimated from photographic photometry and/or spectral type, * the Hipparcos parallax is negative.…”
Section: Input Datamentioning
confidence: 99%
“…Since the discovery of its light variability and its identification as a W UMa‐type eclipsing binary by Shapley & Hughes (1934), the short‐period eclipsing binary BX Pegasi (BX Peg: HV 6149, GSC 02197−01458, RX J213849.2+264121) system has been the subject of several investigations. Reviews of the observational history of the system prior to 1990 appear in Samec (1990) and Samec & Hube (1991). We will now highlight some historical details and also review some work published since 1990.…”
Section: Introductionmentioning
confidence: 99%
“…Several photoelectric and charge‐coupled device (CCD) observations have been made: standardized V and B ones by Zhai & Zhang (1979), Hoffmann (1982) and Samec (1990); V and I data by Samec & Bookmyer (1987); and ‘wide red’ and ‘ v ’ measures by DeYoung, Schmidt & Gritz (1991). Hoffmann's and Samec & Bookmyer's light curves were somewhat incomplete due to poor seeing and instrumental problems, respectively.…”
Section: Introductionmentioning
confidence: 99%
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