Table 5. Open in new tab Diagnostic...

Criteria	[WO1]	[WO2]	[WO3]	WRPN	Classification
Acker & Neiner (2003)
\|$F_\rm{O{\,\small VI}\ 3822}/F_\text{RB}$\|	>1400	1000 ± 200	250 ± 40	822.5 ± 2.6	[WO2]
\|$F_\rm{C{\,\small IV}\ 4650}/F_\text{RB}$\|	300 ± 100	270 ± 60	23 ± 2	149.3 ± 1.7	[WO2]
\|$F_\rm{C{\,\small IV}\ 4686}/F_\text{RB}$\|	500 ± 200	300 ± 30	130 ± 30	170.2 ± 1.7	[WO2–3]
\|$F_\rm{O{\,\small VI}\ 5290}/F_\text{RB}\, ^{\dagger }$\|	>80	48 ± 2	20 ± 5	36.3 ± 0.3	[WO2–3]
\|$F_\rm{C{\,\small IV}\ 5412}/F_\text{RB}$\|	45 ± 15	20 ± 4	15 ± 4	23.5 ± 0.3	[WO2]
\|$F_\rm{C{\,\small IV}\ 5470}/F_\text{RB}$\|	35 ± 5	23 ± 2	14 ± 2	19.1 ± 0.3	[WO2]
\|$F_\rm{Ne{\,\small VII}\ 5666}/F_\text{RB}\, ^{\dagger }$\|	>25	10:	8 ± 6	4.5 ± 0.2	[WO2–3]
\|$F_\rm{Ne{\,\small VIII}\ 6068}/F_\text{RB}\, ^{\dagger }$\|	20 ± 8	6 ± 1	2 ± 1	4.18 ± 0.2	[WO2–3]
\|$F_\rm{O{\,\small V}\ 6740}/F_\text{RB}$\|	Presence	–	–	3.7 ± 0.3	[WO1]
\|$F_\rm{C{\,\small IV}\ 7060}/F_\text{RB}$\|	35 ± 20	18 ± 4	15 ± 4	23.6 ± 0.2	[WO1–2]
FWHM of C iv λλ5806[Å]	33 ± 5	32 ± 3	37 ± 6	37.4	[WO1–3]
Crowther et al. (1998)
log\|$(EW_\rm{O{\,\small VI}3820}/EW_\rm{O{\,\small V}5590})$\|	≥1.1	0.6–1.1	0.25–0.6	1.58	[WO1]
log\|$(EW_\rm{O{\,\small VI}3820}/EW_\rm{C{\,\small IV}5806})$\|	≥0.2	≥0.2	−1–0.2	0.46	[WO1–2]
log\|$(EW_\rm{Ne{\,\small VII}5666}/EW_\rm{O{\,\small V}5590})\, ^{\dagger }$\|	≥0.0	≤0.0	<<0.0	−0.19	[WO2]
FWHM of C iv λλ5806 [Å]	40 ± 10	160 ± 20	90 ± 30	37.4	[WO1]

Criteria

[WO1]

[WO2]

[WO3]

WRPN

Classification

(1)

(2)

(3)

(4)

(5)

(6)

Acker & Neiner (2003)

|$F_\rm{O{\,\small VI}\ 3822}/F_\text{RB}$|

>1400

1000 ± 200

250 ± 40

822.5 ± 2.6

[WO2]

|$F_\rm{C{\,\small IV}\ 4650}/F_\text{RB}$|

300 ± 100

270 ± 60

23 ± 2

149.3 ± 1.7

[WO2]

|$F_\rm{C{\,\small IV}\ 4686}/F_\text{RB}$|

500 ± 200

300 ± 30

130 ± 30

170.2 ± 1.7

[WO2–3]

|$F_\rm{O{\,\small VI}\ 5290}/F_\text{RB}\, ^{\dagger }$|

>80

48 ± 2

20 ± 5

36.3 ± 0.3

[WO2–3]

|$F_\rm{C{\,\small IV}\ 5412}/F_\text{RB}$|

45 ± 15

20 ± 4

15 ± 4

23.5 ± 0.3

[WO2]

|$F_\rm{C{\,\small IV}\ 5470}/F_\text{RB}$|

35 ± 5

23 ± 2

14 ± 2

19.1 ± 0.3

[WO2]

|$F_\rm{Ne{\,\small VII}\ 5666}/F_\text{RB}\, ^{\dagger }$|

>25

10:

8 ± 6

4.5 ± 0.2

[WO2–3]

|$F_\rm{Ne{\,\small VIII}\ 6068}/F_\text{RB}\, ^{\dagger }$|

20 ± 8

6 ± 1

2 ± 1

4.18 ± 0.2

[WO2–3]

|$F_\rm{O{\,\small V}\ 6740}/F_\text{RB}$|

Presence

–

3.7 ± 0.3

[WO1]

|$F_\rm{C{\,\small IV}\ 7060}/F_\text{RB}$|

35 ± 20

18 ± 4

15 ± 4

23.6 ± 0.2

[WO1–2]

FWHM of C iv λλ5806[Å]

33 ± 5

32 ± 3

37 ± 6

37.4

[WO1–3]

Crowther et al. (1998)

log|$(EW_\rm{O{\,\small VI}3820}/EW_\rm{O{\,\small V}5590})$|

≥1.1

0.6–1.1

0.25–0.6

1.58

[WO1]

log|$(EW_\rm{O{\,\small VI}3820}/EW_\rm{C{\,\small IV}5806})$|

≥0.2

−1–0.2

0.46

[WO1–2]

log|$(EW_\rm{Ne{\,\small VII}5666}/EW_\rm{O{\,\small V}5590})\, ^{\dagger }$|

≥0.0

≤0.0

<<0.0

−0.19

[WO2]

FWHM of C iv λλ5806 [Å]

40 ± 10

160 ± 20

90 ± 30

37.4

[WO1]

Criteria	[WO1]	[WO2]	[WO3]	WRPN	Classification
Acker & Neiner (2003)
\|$F_\rm{O{\,\small VI}\ 3822}/F_\text{RB}$\|	>1400	1000 ± 200	250 ± 40	822.5 ± 2.6	[WO2]
\|$F_\rm{C{\,\small IV}\ 4650}/F_\text{RB}$\|	300 ± 100	270 ± 60	23 ± 2	149.3 ± 1.7	[WO2]
\|$F_\rm{C{\,\small IV}\ 4686}/F_\text{RB}$\|	500 ± 200	300 ± 30	130 ± 30	170.2 ± 1.7	[WO2–3]
\|$F_\rm{O{\,\small VI}\ 5290}/F_\text{RB}\, ^{\dagger }$\|	>80	48 ± 2	20 ± 5	36.3 ± 0.3	[WO2–3]
\|$F_\rm{C{\,\small IV}\ 5412}/F_\text{RB}$\|	45 ± 15	20 ± 4	15 ± 4	23.5 ± 0.3	[WO2]
\|$F_\rm{C{\,\small IV}\ 5470}/F_\text{RB}$\|	35 ± 5	23 ± 2	14 ± 2	19.1 ± 0.3	[WO2]
\|$F_\rm{Ne{\,\small VII}\ 5666}/F_\text{RB}\, ^{\dagger }$\|	>25	10:	8 ± 6	4.5 ± 0.2	[WO2–3]
\|$F_\rm{Ne{\,\small VIII}\ 6068}/F_\text{RB}\, ^{\dagger }$\|	20 ± 8	6 ± 1	2 ± 1	4.18 ± 0.2	[WO2–3]
\|$F_\rm{O{\,\small V}\ 6740}/F_\text{RB}$\|	Presence	–	–	3.7 ± 0.3	[WO1]
\|$F_\rm{C{\,\small IV}\ 7060}/F_\text{RB}$\|	35 ± 20	18 ± 4	15 ± 4	23.6 ± 0.2	[WO1–2]
FWHM of C iv λλ5806[Å]	33 ± 5	32 ± 3	37 ± 6	37.4	[WO1–3]
Crowther et al. (1998)
log\|$(EW_\rm{O{\,\small VI}3820}/EW_\rm{O{\,\small V}5590})$\|	≥1.1	0.6–1.1	0.25–0.6	1.58	[WO1]
log\|$(EW_\rm{O{\,\small VI}3820}/EW_\rm{C{\,\small IV}5806})$\|	≥0.2	≥0.2	−1–0.2	0.46	[WO1–2]
log\|$(EW_\rm{Ne{\,\small VII}5666}/EW_\rm{O{\,\small V}5590})\, ^{\dagger }$\|	≥0.0	≤0.0	<<0.0	−0.19	[WO2]
FWHM of C iv λλ5806 [Å]	40 ± 10	160 ± 20	90 ± 30	37.4	[WO1]

Table 5.

Open in new tab

Diagnostic criteria to classify HD 193949 as a [WR]-type CSPN.

Criteria	[WO1]	[WO2]	[WO3]	WRPN	Classification
(1)	(2)	(3)	(4)	(5)	(6)
Acker & Neiner (2003)
\|$F_\rm{O{\,\small VI}\ 3822}/F_\text{RB}$\|	>1400	1000 ± 200	250 ± 40	822.5 ± 2.6	[WO2]
\|$F_\rm{C{\,\small IV}\ 4650}/F_\text{RB}$\|	300 ± 100	270 ± 60	23 ± 2	149.3 ± 1.7	[WO2]
\|$F_\rm{C{\,\small IV}\ 4686}/F_\text{RB}$\|	500 ± 200	300 ± 30	130 ± 30	170.2 ± 1.7	[WO2–3]
\|$F_\rm{O{\,\small VI}\ 5290}/F_\text{RB}\, ^{\dagger }$\|	>80	48 ± 2	20 ± 5	36.3 ± 0.3	[WO2–3]
\|$F_\rm{C{\,\small IV}\ 5412}/F_\text{RB}$\|	45 ± 15	20 ± 4	15 ± 4	23.5 ± 0.3	[WO2]
\|$F_\rm{C{\,\small IV}\ 5470}/F_\text{RB}$\|	35 ± 5	23 ± 2	14 ± 2	19.1 ± 0.3	[WO2]
\|$F_\rm{Ne{\,\small VII}\ 5666}/F_\text{RB}\, ^{\dagger }$\|	>25	10:	8 ± 6	4.5 ± 0.2	[WO2–3]
\|$F_\rm{Ne{\,\small VIII}\ 6068}/F_\text{RB}\, ^{\dagger }$\|	20 ± 8	6 ± 1	2 ± 1	4.18 ± 0.2	[WO2–3]
\|$F_\rm{O{\,\small V}\ 6740}/F_\text{RB}$\|	Presence	–	–	3.7 ± 0.3	[WO1]
\|$F_\rm{C{\,\small IV}\ 7060}/F_\text{RB}$\|	35 ± 20	18 ± 4	15 ± 4	23.6 ± 0.2	[WO1–2]
FWHM of C iv λλ5806[Å]	33 ± 5	32 ± 3	37 ± 6	37.4	[WO1–3]
Crowther et al. (1998)
log\|$(EW_\rm{O{\,\small VI}3820}/EW_\rm{O{\,\small V}5590})$\|	≥1.1	0.6–1.1	0.25–0.6	1.58	[WO1]
log\|$(EW_\rm{O{\,\small VI}3820}/EW_\rm{C{\,\small IV}5806})$\|	≥0.2	≥0.2	−1–0.2	0.46	[WO1–2]
log\|$(EW_\rm{Ne{\,\small VII}5666}/EW_\rm{O{\,\small V}5590})\, ^{\dagger }$\|	≥0.0	≤0.0	<<0.0	−0.19	[WO2]
FWHM of C iv λλ5806 [Å]	40 ± 10	160 ± 20	90 ± 30	37.4	[WO1]

Criteria	[WO1]	[WO2]	[WO3]	WRPN	Classification
(1)	(2)	(3)	(4)	(5)	(6)
Acker & Neiner (2003)
\|$F_\rm{O{\,\small VI}\ 3822}/F_\text{RB}$\|	>1400	1000 ± 200	250 ± 40	822.5 ± 2.6	[WO2]
\|$F_\rm{C{\,\small IV}\ 4650}/F_\text{RB}$\|	300 ± 100	270 ± 60	23 ± 2	149.3 ± 1.7	[WO2]
\|$F_\rm{C{\,\small IV}\ 4686}/F_\text{RB}$\|	500 ± 200	300 ± 30	130 ± 30	170.2 ± 1.7	[WO2–3]
\|$F_\rm{O{\,\small VI}\ 5290}/F_\text{RB}\, ^{\dagger }$\|	>80	48 ± 2	20 ± 5	36.3 ± 0.3	[WO2–3]
\|$F_\rm{C{\,\small IV}\ 5412}/F_\text{RB}$\|	45 ± 15	20 ± 4	15 ± 4	23.5 ± 0.3	[WO2]
\|$F_\rm{C{\,\small IV}\ 5470}/F_\text{RB}$\|	35 ± 5	23 ± 2	14 ± 2	19.1 ± 0.3	[WO2]
\|$F_\rm{Ne{\,\small VII}\ 5666}/F_\text{RB}\, ^{\dagger }$\|	>25	10:	8 ± 6	4.5 ± 0.2	[WO2–3]
\|$F_\rm{Ne{\,\small VIII}\ 6068}/F_\text{RB}\, ^{\dagger }$\|	20 ± 8	6 ± 1	2 ± 1	4.18 ± 0.2	[WO2–3]
\|$F_\rm{O{\,\small V}\ 6740}/F_\text{RB}$\|	Presence	–	–	3.7 ± 0.3	[WO1]
\|$F_\rm{C{\,\small IV}\ 7060}/F_\text{RB}$\|	35 ± 20	18 ± 4	15 ± 4	23.6 ± 0.2	[WO1–2]
FWHM of C iv λλ5806[Å]	33 ± 5	32 ± 3	37 ± 6	37.4	[WO1–3]
Crowther et al. (1998)
log\|$(EW_\rm{O{\,\small VI}3820}/EW_\rm{O{\,\small V}5590})$\|	≥1.1	0.6–1.1	0.25–0.6	1.58	[WO1]
log\|$(EW_\rm{O{\,\small VI}3820}/EW_\rm{C{\,\small IV}5806})$\|	≥0.2	≥0.2	−1–0.2	0.46	[WO1–2]
log\|$(EW_\rm{Ne{\,\small VII}5666}/EW_\rm{O{\,\small V}5590})\, ^{\dagger }$\|	≥0.0	≤0.0	<<0.0	−0.19	[WO2]
FWHM of C iv λλ5806 [Å]	40 ± 10	160 ± 20	90 ± 30	37.4	[WO1]

^†Note that we here identify the λ5290 emission line as O vi and not as C vi; the λ5666 as Ne vii and not as O vii; and the λ6068 as Ne viii and not as O viii, as previously defined (see Crowther et al. 1998; Acker & Neiner 2003). However, according to spectral observations these updated criteria remain as valid as before (see Werner et al. 2007), and given its importance for classification, the re-identification is worth clarifying for future use. See text for details.

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