Table 4. Open in new tab List of...

Name	P	e	Be Sp.type	M(Be)	M_comp	i	Reference
γ Casstars
γ Cas	203.6	0	B0IV	13	0.98*	45	Nemravová et al. (2012)
V782 Cas	122.0	0	B2.5III	9	0.6–0.7*	60–90	this work
HD 45995	103.1	0	B2V	10	1.0 ± 0.1*	46.8	this work
V558 Lyr	83.3	0	B3V	8	0.7–0.8*	60–90	this work
SAO 49725	26.11	0	B0.5III	13	0.2–0.5*	30–90	this work
	137.0	0			0.4–0.7*	30–90	this work
V2156 Cyg	126.6	0	B1.5V	11	0.7–0.8*	60–90	this work
π Aqr	84.1	0	B1V	15	2.4 ± 0.5	70	Bjorkman et al. (2002)
V810 Cas	75.8	0	B1	12.5	0.7–0.8*	60–90	this work
Other Be stars
ϕ Per	126.7	0	B1.5V	9.6	1.2 ± 0.2	77.6	Mourard et al. (2015)
ζ Tau	133.0	0	B1IV	11	0.9–1.0*	60–90	Ruždjak et al. (2009)
HR 2142	80.9	0	B1.5IV-V	10.5	0.7*	85	Peters et al. (2016)
LB-1	78.8	0	B3V	7 ± 2	1.5 ± 0.4*	39	Shenar et al. (2020)
HD 55606	93.8	0	B2.5-3V	6.0–6.6	0.83–0.9	75–85	Chojnowski et al. (2018)
FY CMa	37.3	0	B0.5IV	10–13	1.1–1.5	>66	Peters et al. (2008)
o Pup	28.9	0	B1IV	11–15	0.7–1.0⁺		Koubský et al. (2012)
MX Pup	5.15	0.46	B1.5III	15	0.6–6.6	5–50	Carrier, Burki & Burnet (2002)
χ Oph	138.8	0.44	B2V	10	1.7–2*	60–90	Abt & Levy (1978)
HD 161306	99.9	0	B0	15	0.9⁺		Koubský et al. (2014)
HR 6819	40.3	0.04	B2.5V	6	0.4–0.8*	35	Gies & Wang (2020)
59 Cyg	28.2	0.14	B1.5V	6.3–9.4	0.6–0.9	60–80	Peters et al. (2013)
60 Cyg	146.6	0	B1V	11.8	1.5–3.4	>29	Koubský et al. (2000)

Name

Be Sp.type

M(Be)

M_comp

Reference

(d)

(M_⊙)

(°)

γ Casstars

γ Cas

203.6

B0IV

0.98*

Nemravová et al. (2012)

V782 Cas

122.0

B2.5III

0.6–0.7*

60–90

this work

HD 45995

103.1

B2V

1.0 ± 0.1*

46.8

this work

V558 Lyr

83.3

B3V

0.7–0.8*

60–90

this work

SAO 49725

26.11

B0.5III

0.2–0.5*

30–90

this work

137.0

0.4–0.7*

30–90

this work

V2156 Cyg

126.6

B1.5V

0.7–0.8*

60–90

this work

π Aqr

84.1

B1V

2.4 ± 0.5

Bjorkman et al. (2002)

V810 Cas

75.8

12.5

0.7–0.8*

60–90

this work

Other Be stars

ϕ Per

126.7

B1.5V

9.6

1.2 ± 0.2

77.6

Mourard et al. (2015)

ζ Tau

133.0

B1IV

0.9–1.0*

60–90

Ruždjak et al. (2009)

HR 2142

80.9

B1.5IV-V

10.5

0.7*

Peters et al. (2016)

LB-1

78.8

B3V

7 ± 2

1.5 ± 0.4*

Shenar et al. (2020)

HD 55606

93.8

B2.5-3V

6.0–6.6

0.83–0.9

75–85

Chojnowski et al. (2018)

FY CMa

37.3

B0.5IV

10–13

1.1–1.5

>66

Peters et al. (2008)

o Pup

28.9

B1IV

11–15

0.7–1.0⁺

Koubský et al. (2012)

MX Pup

5.15

0.46

B1.5III

0.6–6.6

5–50

Carrier, Burki & Burnet (2002)

χ Oph

138.8

0.44

B2V

1.7–2*

60–90

Abt & Levy (1978)

HD 161306

99.9

0.9⁺

Koubský et al. (2014)

HR 6819

40.3

0.04

B2.5V

0.4–0.8*

Gies & Wang (2020)

59 Cyg

28.2

0.14

B1.5V

6.3–9.4

0.6–0.9

60–80

Peters et al. (2013)

60 Cyg

146.6

B1V

11.8

1.5–3.4

>29

Koubský et al. (2000)

Name	P	e	Be Sp.type	M(Be)	M_comp	i	Reference
γ Casstars
γ Cas	203.6	0	B0IV	13	0.98*	45	Nemravová et al. (2012)
V782 Cas	122.0	0	B2.5III	9	0.6–0.7*	60–90	this work
HD 45995	103.1	0	B2V	10	1.0 ± 0.1*	46.8	this work
V558 Lyr	83.3	0	B3V	8	0.7–0.8*	60–90	this work
SAO 49725	26.11	0	B0.5III	13	0.2–0.5*	30–90	this work
	137.0	0			0.4–0.7*	30–90	this work
V2156 Cyg	126.6	0	B1.5V	11	0.7–0.8*	60–90	this work
π Aqr	84.1	0	B1V	15	2.4 ± 0.5	70	Bjorkman et al. (2002)
V810 Cas	75.8	0	B1	12.5	0.7–0.8*	60–90	this work
Other Be stars
ϕ Per	126.7	0	B1.5V	9.6	1.2 ± 0.2	77.6	Mourard et al. (2015)
ζ Tau	133.0	0	B1IV	11	0.9–1.0*	60–90	Ruždjak et al. (2009)
HR 2142	80.9	0	B1.5IV-V	10.5	0.7*	85	Peters et al. (2016)
LB-1	78.8	0	B3V	7 ± 2	1.5 ± 0.4*	39	Shenar et al. (2020)
HD 55606	93.8	0	B2.5-3V	6.0–6.6	0.83–0.9	75–85	Chojnowski et al. (2018)
FY CMa	37.3	0	B0.5IV	10–13	1.1–1.5	>66	Peters et al. (2008)
o Pup	28.9	0	B1IV	11–15	0.7–1.0⁺		Koubský et al. (2012)
MX Pup	5.15	0.46	B1.5III	15	0.6–6.6	5–50	Carrier, Burki & Burnet (2002)
χ Oph	138.8	0.44	B2V	10	1.7–2*	60–90	Abt & Levy (1978)
HD 161306	99.9	0	B0	15	0.9⁺		Koubský et al. (2014)
HR 6819	40.3	0.04	B2.5V	6	0.4–0.8*	35	Gies & Wang (2020)
59 Cyg	28.2	0.14	B1.5V	6.3–9.4	0.6–0.9	60–80	Peters et al. (2013)
60 Cyg	146.6	0	B1V	11.8	1.5–3.4	>29	Koubský et al. (2000)

Table 4.

Open in new tab

List of binaries with an early (B0–3) classical Be primary and an existing orbital solution, ordered by right ascension (R.A.).

Name	P	e	Be Sp.type	M(Be)	M_comp	i	Reference
	(d)			(M_⊙)	(M_⊙)	(°)
γ Casstars
γ Cas	203.6	0	B0IV	13	0.98*	45	Nemravová et al. (2012)
V782 Cas	122.0	0	B2.5III	9	0.6–0.7*	60–90	this work
HD 45995	103.1	0	B2V	10	1.0 ± 0.1*	46.8	this work
V558 Lyr	83.3	0	B3V	8	0.7–0.8*	60–90	this work
SAO 49725	26.11	0	B0.5III	13	0.2–0.5*	30–90	this work
	137.0	0			0.4–0.7*	30–90	this work
V2156 Cyg	126.6	0	B1.5V	11	0.7–0.8*	60–90	this work
π Aqr	84.1	0	B1V	15	2.4 ± 0.5	70	Bjorkman et al. (2002)
V810 Cas	75.8	0	B1	12.5	0.7–0.8*	60–90	this work
Other Be stars
ϕ Per	126.7	0	B1.5V	9.6	1.2 ± 0.2	77.6	Mourard et al. (2015)
ζ Tau	133.0	0	B1IV	11	0.9–1.0*	60–90	Ruždjak et al. (2009)
HR 2142	80.9	0	B1.5IV-V	10.5	0.7*	85	Peters et al. (2016)
LB-1	78.8	0	B3V	7 ± 2	1.5 ± 0.4*	39	Shenar et al. (2020)
HD 55606	93.8	0	B2.5-3V	6.0–6.6	0.83–0.9	75–85	Chojnowski et al. (2018)
FY CMa	37.3	0	B0.5IV	10–13	1.1–1.5	>66	Peters et al. (2008)
o Pup	28.9	0	B1IV	11–15	0.7–1.0⁺		Koubský et al. (2012)
MX Pup	5.15	0.46	B1.5III	15	0.6–6.6	5–50	Carrier, Burki & Burnet (2002)
χ Oph	138.8	0.44	B2V	10	1.7–2*	60–90	Abt & Levy (1978)
HD 161306	99.9	0	B0	15	0.9⁺		Koubský et al. (2014)
HR 6819	40.3	0.04	B2.5V	6	0.4–0.8*	35	Gies & Wang (2020)
59 Cyg	28.2	0.14	B1.5V	6.3–9.4	0.6–0.9	60–80	Peters et al. (2013)
60 Cyg	146.6	0	B1V	11.8	1.5–3.4	>29	Koubský et al. (2000)

Name	P	e	Be Sp.type	M(Be)	M_comp	i	Reference
	(d)			(M_⊙)	(M_⊙)	(°)
γ Casstars
γ Cas	203.6	0	B0IV	13	0.98*	45	Nemravová et al. (2012)
V782 Cas	122.0	0	B2.5III	9	0.6–0.7*	60–90	this work
HD 45995	103.1	0	B2V	10	1.0 ± 0.1*	46.8	this work
V558 Lyr	83.3	0	B3V	8	0.7–0.8*	60–90	this work
SAO 49725	26.11	0	B0.5III	13	0.2–0.5*	30–90	this work
	137.0	0			0.4–0.7*	30–90	this work
V2156 Cyg	126.6	0	B1.5V	11	0.7–0.8*	60–90	this work
π Aqr	84.1	0	B1V	15	2.4 ± 0.5	70	Bjorkman et al. (2002)
V810 Cas	75.8	0	B1	12.5	0.7–0.8*	60–90	this work
Other Be stars
ϕ Per	126.7	0	B1.5V	9.6	1.2 ± 0.2	77.6	Mourard et al. (2015)
ζ Tau	133.0	0	B1IV	11	0.9–1.0*	60–90	Ruždjak et al. (2009)
HR 2142	80.9	0	B1.5IV-V	10.5	0.7*	85	Peters et al. (2016)
LB-1	78.8	0	B3V	7 ± 2	1.5 ± 0.4*	39	Shenar et al. (2020)
HD 55606	93.8	0	B2.5-3V	6.0–6.6	0.83–0.9	75–85	Chojnowski et al. (2018)
FY CMa	37.3	0	B0.5IV	10–13	1.1–1.5	>66	Peters et al. (2008)
o Pup	28.9	0	B1IV	11–15	0.7–1.0⁺		Koubský et al. (2012)
MX Pup	5.15	0.46	B1.5III	15	0.6–6.6	5–50	Carrier, Burki & Burnet (2002)
χ Oph	138.8	0.44	B2V	10	1.7–2*	60–90	Abt & Levy (1978)
HD 161306	99.9	0	B0	15	0.9⁺		Koubský et al. (2014)
HR 6819	40.3	0.04	B2.5V	6	0.4–0.8*	35	Gies & Wang (2020)
59 Cyg	28.2	0.14	B1.5V	6.3–9.4	0.6–0.9	60–80	Peters et al. (2013)
60 Cyg	146.6	0	B1V	11.8	1.5–3.4	>29	Koubský et al. (2000)

Notes. * indicates SB1 systems for which the secondary mass was estimated from the probable values of primary mass, mass function, and inclination. ⁺ indicates SB2 systems for which the secondary mass was estimated from the mass ratio (derived from velocity amplitudes) and a probable value of the primary mass. When unconstrained, inclination is taken to be 60–90°. Note that, for γ Cas, the results of Smith et al. (2012) and Nemravová et al. (2012) are similar – only the latter is quoted here. Velocity shifts have also been recorded for the secondary in HD 194335, although a full orbital coverage has not yet been acquired (Wang et al. 2021), hence we do not yet add it to this Table.

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