1997
DOI: 10.1086/118553
|View full text |Cite
|
Sign up to set email alerts
|

Absolute dimensions and masses of IT cassiopeiae.

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

1
12
0

Year Published

2000
2000
2012
2012

Publication Types

Select...
8

Relationship

0
8

Authors

Journals

citations
Cited by 19 publications
(13 citation statements)
references
References 0 publications
1
12
0
Order By: Relevance
“…5 and 6 and is denoted by a star. However, we did not consider this system in our present investigation since there seems to be a discrepancy in its observed apsidal-motion rate (Lacy et al 1997;Kozyreva & Zakharov 2001). …”
Section: Comparison With Observationsmentioning
confidence: 95%
“…5 and 6 and is denoted by a star. However, we did not consider this system in our present investigation since there seems to be a discrepancy in its observed apsidal-motion rate (Lacy et al 1997;Kozyreva & Zakharov 2001). …”
Section: Comparison With Observationsmentioning
confidence: 95%
“…See also history summarized in that paper. Accurate masses and radii was determined spectroscopically by Lacy et al (1997), who detected components of similar mass and size (see Table 3). They also excluded the previous reports of δ Scuti variations.…”
Section: It Casmentioning
confidence: 99%
“…Apart from the minima given in Table A.1, we add numerous times of minimum obtained by several observers: Lacy et al (1997, their Table 4, 1998), Agerer & Hübscher (2003), Diethelm (2003), Nakajima (2003) 3 , Hübscher (2005), Hübscher et al (2005), Smith & Caton (2007), and Hübscher & Walter (2007). A total of 95 times of minimum are now available, of which 51 correspond to primary eclipses and 44 to secondary eclipses (Table A.2).…”
Section: It Casmentioning
confidence: 99%
“…The occurrence of a third object in the system of GSC 3822-1056 is not unprecedented, but it has relatively high luminosity compared to the close pair. Note that V909 Cygni (although it is an Algol-star object) also has high fractional luminosity third companion (in that case L 3 /L total ≈ 0.22 in B and V, Lacy et al 1999). Other Algols, as AC Vel (10-15% third light in y, Johanssen et al 1997) and DI Peg (22-25% third light in V, Rucinski 1967) also have large third light.…”
Section: Light Curve Solutionmentioning
confidence: 99%