Table 2. Open in new tab Orbital periods...

Nova

Year

D (pc)

E(B − V)

|$M_{\rm WD}^a$|

|$M_{\rm comp}^b$|

SED^c

T_comp (K)

F₀ (mJy)

R_comp (R_⊙)

P(d)

T CrB

S(6)

920 ± 20

0.06 ± 0.04

1.35

1.08

GAP2W

2830 ± 70

6370 ± 400

88.6 ± 2.8

287 ± 27

V1330 Cyg

1970

S(217)

2900 ± 600

0.3 ± 0.1

0.91

0.73

GZP2W

6050 ± 220

1.0 ± 0.1

1.12 ± 0.25

0.50 ± 0.17

RS Oph

P(14)

2700 ± 140

0.65 ± 0.10

1.33

1.06

GAP2W

3630 ± 130

2110 ± 16

103 ± 7

365 ± 52

V794 Oph

1939

J(220)

8000 ± 1000

0.9 ± 0.1

0.85

0.68

RZP2

4530 ± 210

6.3 ± 1

12.0 ± 2.1

18.0 ± 4.8

V3664 Oph

2018

...

8000 ± 1000

0.72 ± 0.2

1.05

0.84

AP2W

2100 ± 50

450 ± 20

320 ± 50

2250 ± 500

GK Per

1901

O(13)

430 ± 10

0.30 ± 0.04

1.22

0.98

GAP2W

3830 ± 100

70.1 ± 2.2

2.76 ± 0.15

1.66 ± 0.14

V392 Per

2018

P(11)

3600 ± 600

0.72 ± 0.15

1.30

1.04

GAP2W

6100 ± 330

7.5 ± 0.2

3.7 ± 0.9

2.6 ± 0.9

KY Sgr

1926

S(109)

8000 ± 1000

1.0 ± 0.5

1.20

0.96

PMV2W

2350 ± 40

46 ± 9

86 ± 12

294 ± 61

V1016 Sgr

1899

S(140)

2600 ± 140

0.35 ± 0.04

1.20

0.96

AP2W

4550 ± 130

51.5 ± 3.6

11.0 ± 0.9

13.4 ± 1.7

V1017 Sgr

1919

S(130)

1200 ± 30

0.25 ± 0.10

1.20

0.96

GLSP2W

4720 ± 150

48 ± 8

4.6 ± 0.5

3.7 ± 0.6

V1172 Sgr

1951

...

8000 ± 1000

0.4 ± 0.1

1.10

0.88

2310 ± 70

34.1 ± 3.9

76.5 ± 12.8

255 ± 64

V3645 Sgr

1970

...

8000 ± 1000

0.39 ± 0.03

1.10

0.88

AP2W

3490 ± 110

9.8 ± 0.5

22.0 ± 3.1

39.5 ± 8.4

V3890 Sgr

S(14)

8000 ± 1000

0.59 ± 0.1

1.38

1.05

ACP2W

2230 ± 60

260 ± 12

223 ± 30

1220 ± 250

V5580 Sgr

2008

...

8000 ± 1000

0.34 ± 0.1

1.10

0.88

AP2W

3900 ± 280

11 ± 1

20 ± 4

34 ± 9

V5581 Sgr

2009

...

8000 ± 1000

1.5 ± 0.3

1.10

0.88

SP2W

2250 ± 60

380 ± 120

266 ± 58

1660 ± 530

V723 Sco

1952

S(23)

8000 ± 1000

0.57 ± 0.10

1.38

1.10

3840 ± 190

1.6 ± 0.2

7.6 ± 1.2

7.2 ± 1.8

V745 Sco

P(9)

8000 ± 1000

1.0 ± 0.2

1.39

1.11

GS2W

2020 ± 60

540 ± 20

370 ± 50

2440 ± 500

V977 Sco

1989

...

8000 ± 1000

0.92 ± 0.10

1.10

0.88

3740 ± 240

6.9 ± 0.8

16.8 ± 3.2

26.2 ± 7.4

V1313 Sco

2011

S(18)

3100 ± 1600

1.00 ± 0.2

1.20

0.96

GS2W

3140 ± 90

70 ± 2

27 ± 13

50 ± 35

V1534 Sco

2014

S(9)

8000 ± 1000

0.92 ± 0.10

1.37

1.10

S2W

2420 ± 80

118 ± 8

133 ± 21

520 ± 120

V1535 Sco

2015

S(20)

8000 ± 1000

0.8 ± 0.2

0.85

0.68

GSA2W

3610 ± 170

12.5 ± 2.2

23.7 ± 4.7

50 ± 14

V1657 Sco

2017

...

8000 ± 1000

1.0 ± 0.1

1.10

0.88

S2W

2870 ± 90

226 ± 26

142 ± 21

650 ± 145

EU Sct

1949

S(42)

5100 ± 1500

0.84 ± 0.10

1.20

0.96

SP2W

3150 ± 110

39 ± 3

32.7 ± 9.7

68 ± 30

FS Sct

1952

J(86)

3600 ± 1500

0.5 ± 0.1

1.00

0.80

PR2W

3170 ± 190

2.6 ± 0.2

5.9 ± 2.6

5.7 ± 3.7

X Ser

1903

S(730)

5100 ± 2000

0.2 ± 0.1

1.05

0.84

GAP2W

5380 ± 320

1.09 ± 0.03

2.45 ± 1.01

1.5 ± 0.9

Nova

Year

D (pc)

E(B − V)

|$M_{\rm WD}^a$|

|$M_{\rm comp}^b$|

SED^c

T_comp (K)

F₀ (mJy)

R_comp (R_⊙)

P(d)

T CrB

S(6)

920 ± 20

0.06 ± 0.04

1.35

1.08

GAP2W

2830 ± 70

6370 ± 400

88.6 ± 2.8

287 ± 27

V1330 Cyg

1970

S(217)

2900 ± 600

0.3 ± 0.1

0.91

0.73

GZP2W

6050 ± 220

1.0 ± 0.1

1.12 ± 0.25

0.50 ± 0.17

RS Oph

P(14)

2700 ± 140

0.65 ± 0.10

1.33

1.06

GAP2W

3630 ± 130

2110 ± 16

103 ± 7

365 ± 52

V794 Oph

1939

J(220)

8000 ± 1000

0.9 ± 0.1

0.85

0.68

RZP2

4530 ± 210

6.3 ± 1

12.0 ± 2.1

18.0 ± 4.8

V3664 Oph

2018

...

8000 ± 1000

0.72 ± 0.2

1.05

0.84

AP2W

2100 ± 50

450 ± 20

320 ± 50

2250 ± 500

GK Per

1901

O(13)

430 ± 10

0.30 ± 0.04

1.22

0.98

GAP2W

3830 ± 100

70.1 ± 2.2

2.76 ± 0.15

1.66 ± 0.14

V392 Per

2018

P(11)

3600 ± 600

0.72 ± 0.15

1.30

1.04

GAP2W

6100 ± 330

7.5 ± 0.2

3.7 ± 0.9

2.6 ± 0.9

KY Sgr

1926

S(109)

8000 ± 1000

1.0 ± 0.5

1.20

0.96

PMV2W

2350 ± 40

46 ± 9

86 ± 12

294 ± 61

V1016 Sgr

1899

S(140)

2600 ± 140

0.35 ± 0.04

1.20

0.96

AP2W

4550 ± 130

51.5 ± 3.6

11.0 ± 0.9

13.4 ± 1.7

V1017 Sgr

1919

S(130)

1200 ± 30

0.25 ± 0.10

1.20

0.96

GLSP2W

4720 ± 150

48 ± 8

4.6 ± 0.5

3.7 ± 0.6

V1172 Sgr

1951

...

8000 ± 1000

0.4 ± 0.1

1.10

0.88

2310 ± 70

34.1 ± 3.9

76.5 ± 12.8

255 ± 64

V3645 Sgr

1970

...

8000 ± 1000

0.39 ± 0.03

1.10

0.88

AP2W

3490 ± 110

9.8 ± 0.5

22.0 ± 3.1

39.5 ± 8.4

V3890 Sgr

S(14)

8000 ± 1000

0.59 ± 0.1

1.38

1.05

ACP2W

2230 ± 60

260 ± 12

223 ± 30

1220 ± 250

V5580 Sgr

2008

...

8000 ± 1000

0.34 ± 0.1

1.10

0.88

AP2W

3900 ± 280

11 ± 1

20 ± 4

34 ± 9

V5581 Sgr

2009

...

8000 ± 1000

1.5 ± 0.3

1.10

0.88

SP2W

2250 ± 60

380 ± 120

266 ± 58

1660 ± 530

V723 Sco

1952

S(23)

8000 ± 1000

0.57 ± 0.10

1.38

1.10

3840 ± 190

1.6 ± 0.2

7.6 ± 1.2

7.2 ± 1.8

V745 Sco

P(9)

8000 ± 1000

1.0 ± 0.2

1.39

1.11

GS2W

2020 ± 60

540 ± 20

370 ± 50

2440 ± 500

V977 Sco

1989

...

8000 ± 1000

0.92 ± 0.10

1.10

0.88

3740 ± 240

6.9 ± 0.8

16.8 ± 3.2

26.2 ± 7.4

V1313 Sco

2011

S(18)

3100 ± 1600

1.00 ± 0.2

1.20

0.96

GS2W

3140 ± 90

70 ± 2

27 ± 13

50 ± 35

V1534 Sco

2014

S(9)

8000 ± 1000

0.92 ± 0.10

1.37

1.10

S2W

2420 ± 80

118 ± 8

133 ± 21

520 ± 120

V1535 Sco

2015

S(20)

8000 ± 1000

0.8 ± 0.2

0.85

0.68

GSA2W

3610 ± 170

12.5 ± 2.2

23.7 ± 4.7

50 ± 14

V1657 Sco

2017

...

8000 ± 1000

1.0 ± 0.1

1.10

0.88

S2W

2870 ± 90

226 ± 26

142 ± 21

650 ± 145

EU Sct

1949

S(42)

5100 ± 1500

0.84 ± 0.10

1.20

0.96

SP2W

3150 ± 110

39 ± 3

32.7 ± 9.7

68 ± 30

FS Sct

1952

J(86)

3600 ± 1500

0.5 ± 0.1

1.00

0.80

PR2W

3170 ± 190

2.6 ± 0.2

5.9 ± 2.6

5.7 ± 3.7

X Ser

1903

S(730)

5100 ± 2000

0.2 ± 0.1

1.05

0.84

GAP2W

5380 ± 320

1.09 ± 0.03

2.45 ± 1.01

1.5 ± 0.9

Table 2.

Open in new tab

Orbital periods measured from SEDs and the blackbody radii.

Nova	Year	LC	D (pc)	E(B − V)	\|$M_{\rm WD}^a$\|	\|$M_{\rm comp}^b$\|	SED^c	T_comp (K)	F₀ (mJy)	R_comp (R_⊙)	P(d)
T CrB	RN	S(6)	920 ± 20	0.06 ± 0.04	1.35	1.08	GAP2W	2830 ± 70	6370 ± 400	88.6 ± 2.8	287 ± 27
V1330 Cyg	1970	S(217)	2900 ± 600	0.3 ± 0.1	0.91	0.73	GZP2W	6050 ± 220	1.0 ± 0.1	1.12 ± 0.25	0.50 ± 0.17
RS Oph	RN	P(14)	2700 ± 140	0.65 ± 0.10	1.33	1.06	GAP2W	3630 ± 130	2110 ± 16	103 ± 7	365 ± 52
V794 Oph	1939	J(220)	8000 ± 1000	0.9 ± 0.1	0.85	0.68	RZP2	4530 ± 210	6.3 ± 1	12.0 ± 2.1	18.0 ± 4.8
V3664 Oph	2018	...	8000 ± 1000	0.72 ± 0.2	1.05	0.84	AP2W	2100 ± 50	450 ± 20	320 ± 50	2250 ± 500
GK Per	1901	O(13)	430 ± 10	0.30 ± 0.04	1.22	0.98	GAP2W	3830 ± 100	70.1 ± 2.2	2.76 ± 0.15	1.66 ± 0.14
V392 Per	2018	P(11)	3600 ± 600	0.72 ± 0.15	1.30	1.04	GAP2W	6100 ± 330	7.5 ± 0.2	3.7 ± 0.9	2.6 ± 0.9
KY Sgr	1926	S(109)	8000 ± 1000	1.0 ± 0.5	1.20	0.96	PMV2W	2350 ± 40	46 ± 9	86 ± 12	294 ± 61
V1016 Sgr	1899	S(140)	2600 ± 140	0.35 ± 0.04	1.20	0.96	AP2W	4550 ± 130	51.5 ± 3.6	11.0 ± 0.9	13.4 ± 1.7
V1017 Sgr	1919	S(130)	1200 ± 30	0.25 ± 0.10	1.20	0.96	GLSP2W	4720 ± 150	48 ± 8	4.6 ± 0.5	3.7 ± 0.6
V1172 Sgr	1951	...	8000 ± 1000	0.4 ± 0.1	1.10	0.88	SW	2310 ± 70	34.1 ± 3.9	76.5 ± 12.8	255 ± 64
V3645 Sgr	1970	...	8000 ± 1000	0.39 ± 0.03	1.10	0.88	AP2W	3490 ± 110	9.8 ± 0.5	22.0 ± 3.1	39.5 ± 8.4
V3890 Sgr	RN	S(14)	8000 ± 1000	0.59 ± 0.1	1.38	1.05	ACP2W	2230 ± 60	260 ± 12	223 ± 30	1220 ± 250
V5580 Sgr	2008	...	8000 ± 1000	0.34 ± 0.1	1.10	0.88	AP2W	3900 ± 280	11 ± 1	20 ± 4	34 ± 9
V5581 Sgr	2009	...	8000 ± 1000	1.5 ± 0.3	1.10	0.88	SP2W	2250 ± 60	380 ± 120	266 ± 58	1660 ± 530
V723 Sco	1952	S(23)	8000 ± 1000	0.57 ± 0.10	1.38	1.10	MV	3840 ± 190	1.6 ± 0.2	7.6 ± 1.2	7.2 ± 1.8
V745 Sco	RN	P(9)	8000 ± 1000	1.0 ± 0.2	1.39	1.11	GS2W	2020 ± 60	540 ± 20	370 ± 50	2440 ± 500
V977 Sco	1989	...	8000 ± 1000	0.92 ± 0.10	1.10	0.88	MV	3740 ± 240	6.9 ± 0.8	16.8 ± 3.2	26.2 ± 7.4
V1313 Sco	2011	S(18)	3100 ± 1600	1.00 ± 0.2	1.20	0.96	GS2W	3140 ± 90	70 ± 2	27 ± 13	50 ± 35
V1534 Sco	2014	S(9)	8000 ± 1000	0.92 ± 0.10	1.37	1.10	S2W	2420 ± 80	118 ± 8	133 ± 21	520 ± 120
V1535 Sco	2015	S(20)	8000 ± 1000	0.8 ± 0.2	0.85	0.68	GSA2W	3610 ± 170	12.5 ± 2.2	23.7 ± 4.7	50 ± 14
V1657 Sco	2017	...	8000 ± 1000	1.0 ± 0.1	1.10	0.88	S2W	2870 ± 90	226 ± 26	142 ± 21	650 ± 145
EU Sct	1949	S(42)	5100 ± 1500	0.84 ± 0.10	1.20	0.96	SP2W	3150 ± 110	39 ± 3	32.7 ± 9.7	68 ± 30
FS Sct	1952	J(86)	3600 ± 1500	0.5 ± 0.1	1.00	0.80	PR2W	3170 ± 190	2.6 ± 0.2	5.9 ± 2.6	5.7 ± 3.7
X Ser	1903	S(730)	5100 ± 2000	0.2 ± 0.1	1.05	0.84	GAP2W	5380 ± 320	1.09 ± 0.03	2.45 ± 1.01	1.5 ± 0.9

Nova	Year	LC	D (pc)	E(B − V)	\|$M_{\rm WD}^a$\|	\|$M_{\rm comp}^b$\|	SED^c	T_comp (K)	F₀ (mJy)	R_comp (R_⊙)	P(d)
T CrB	RN	S(6)	920 ± 20	0.06 ± 0.04	1.35	1.08	GAP2W	2830 ± 70	6370 ± 400	88.6 ± 2.8	287 ± 27
V1330 Cyg	1970	S(217)	2900 ± 600	0.3 ± 0.1	0.91	0.73	GZP2W	6050 ± 220	1.0 ± 0.1	1.12 ± 0.25	0.50 ± 0.17
RS Oph	RN	P(14)	2700 ± 140	0.65 ± 0.10	1.33	1.06	GAP2W	3630 ± 130	2110 ± 16	103 ± 7	365 ± 52
V794 Oph	1939	J(220)	8000 ± 1000	0.9 ± 0.1	0.85	0.68	RZP2	4530 ± 210	6.3 ± 1	12.0 ± 2.1	18.0 ± 4.8
V3664 Oph	2018	...	8000 ± 1000	0.72 ± 0.2	1.05	0.84	AP2W	2100 ± 50	450 ± 20	320 ± 50	2250 ± 500
GK Per	1901	O(13)	430 ± 10	0.30 ± 0.04	1.22	0.98	GAP2W	3830 ± 100	70.1 ± 2.2	2.76 ± 0.15	1.66 ± 0.14
V392 Per	2018	P(11)	3600 ± 600	0.72 ± 0.15	1.30	1.04	GAP2W	6100 ± 330	7.5 ± 0.2	3.7 ± 0.9	2.6 ± 0.9
KY Sgr	1926	S(109)	8000 ± 1000	1.0 ± 0.5	1.20	0.96	PMV2W	2350 ± 40	46 ± 9	86 ± 12	294 ± 61
V1016 Sgr	1899	S(140)	2600 ± 140	0.35 ± 0.04	1.20	0.96	AP2W	4550 ± 130	51.5 ± 3.6	11.0 ± 0.9	13.4 ± 1.7
V1017 Sgr	1919	S(130)	1200 ± 30	0.25 ± 0.10	1.20	0.96	GLSP2W	4720 ± 150	48 ± 8	4.6 ± 0.5	3.7 ± 0.6
V1172 Sgr	1951	...	8000 ± 1000	0.4 ± 0.1	1.10	0.88	SW	2310 ± 70	34.1 ± 3.9	76.5 ± 12.8	255 ± 64
V3645 Sgr	1970	...	8000 ± 1000	0.39 ± 0.03	1.10	0.88	AP2W	3490 ± 110	9.8 ± 0.5	22.0 ± 3.1	39.5 ± 8.4
V3890 Sgr	RN	S(14)	8000 ± 1000	0.59 ± 0.1	1.38	1.05	ACP2W	2230 ± 60	260 ± 12	223 ± 30	1220 ± 250
V5580 Sgr	2008	...	8000 ± 1000	0.34 ± 0.1	1.10	0.88	AP2W	3900 ± 280	11 ± 1	20 ± 4	34 ± 9
V5581 Sgr	2009	...	8000 ± 1000	1.5 ± 0.3	1.10	0.88	SP2W	2250 ± 60	380 ± 120	266 ± 58	1660 ± 530
V723 Sco	1952	S(23)	8000 ± 1000	0.57 ± 0.10	1.38	1.10	MV	3840 ± 190	1.6 ± 0.2	7.6 ± 1.2	7.2 ± 1.8
V745 Sco	RN	P(9)	8000 ± 1000	1.0 ± 0.2	1.39	1.11	GS2W	2020 ± 60	540 ± 20	370 ± 50	2440 ± 500
V977 Sco	1989	...	8000 ± 1000	0.92 ± 0.10	1.10	0.88	MV	3740 ± 240	6.9 ± 0.8	16.8 ± 3.2	26.2 ± 7.4
V1313 Sco	2011	S(18)	3100 ± 1600	1.00 ± 0.2	1.20	0.96	GS2W	3140 ± 90	70 ± 2	27 ± 13	50 ± 35
V1534 Sco	2014	S(9)	8000 ± 1000	0.92 ± 0.10	1.37	1.10	S2W	2420 ± 80	118 ± 8	133 ± 21	520 ± 120
V1535 Sco	2015	S(20)	8000 ± 1000	0.8 ± 0.2	0.85	0.68	GSA2W	3610 ± 170	12.5 ± 2.2	23.7 ± 4.7	50 ± 14
V1657 Sco	2017	...	8000 ± 1000	1.0 ± 0.1	1.10	0.88	S2W	2870 ± 90	226 ± 26	142 ± 21	650 ± 145
EU Sct	1949	S(42)	5100 ± 1500	0.84 ± 0.10	1.20	0.96	SP2W	3150 ± 110	39 ± 3	32.7 ± 9.7	68 ± 30
FS Sct	1952	J(86)	3600 ± 1500	0.5 ± 0.1	1.00	0.80	PR2W	3170 ± 190	2.6 ± 0.2	5.9 ± 2.6	5.7 ± 3.7
X Ser	1903	S(730)	5100 ± 2000	0.2 ± 0.1	1.05	0.84	GAP2W	5380 ± 320	1.09 ± 0.03	2.45 ± 1.01	1.5 ± 0.9

The white dwarf mass is in units of M_⊙. The error bars are near 0.03 M_⊙ for the RNe, and estimated as 0.10–0.20 M_⊙ for the other novae. The size of these error bars are negligible for the uncertainty in P.

The companion mass is in units of M_⊙. The error bars are always poorly known, estimated to be 0.10–0.20 M_⊙, and negligible for contributing to the uncertainty in P.

The sources for the SEDs are indicated with a letter or number: A – AAVSO (including APASS), C – Schaefer (2010), G – Galex, L – Landolt (2016), M – Mróz et al. (2015), P – Pan-STARRS, R – Ringwald, Naylor & Mukai et al. (1996), S – SMARTS, V – Saito et al. (2013), W – Wise, Z – Szkody (1994), and 2 – 2MASS.

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