Table 5
Line equivalent widths and line fluxes for hydrogen and helium lines.
Hydrogen lines | Helium lines | |||||||||||
ID name | E W Hα | log FHα | E W Hβ | log FHβ | E W λ5876 | log Fλ5876 | E W λ6678 | log Fλ6678 | E W λ7065 | log Fλ7065 | accretor | notes |
(Å) | (erg s-1 cm2) | (Å) | (erg s-1 cm2) | (Å) | (erg s-1 cm2) | (Å) | (erg s-1 cm2) | (Å) | (erg s-1 cm2) | (Y/N) | ||
|
||||||||||||
RXS J045912.4−033711 | 1.80 ± 0.20 | ... | N | G | ||||||||
1RXS J050416.9−021426 | 0.03 ± 0.20 | ... | N | G | ||||||||
TTS J050513.5−034248 | −9.80 ± 0.40 | 6.2 | N | G | ||||||||
TTS J050538.9−032626 | −4.90 ± 0.20 | 6.2 | N | G | ||||||||
RX J0506.6−0337 | 1.00 ± 0.20 | ... | N | G | ||||||||
TTS J050644.4−032913 | −4.70 ± 0.30 | 6.0 | N | G | ||||||||
TTS J050646.1−031922 | −35.2 ± 0.8 | 8.0 | ... | ... | ... | ... | Y | |||||
−34.8 ± 1.5 | 8.0 | ... | ... | ... | ... | |||||||
RX J0506.8−0318 | −1.3 ± 0.1 | 6.1 | ... | ... | ... | ... | N | |||||
−1.2 ± 0.1 | 6.1 | ... | ... | ... | ... | |||||||
−1.5 ± 0.1 | 6.2 | ... | ... | ... | ... | |||||||
TTS J050647.5−031910 | −0.7 ± 0.1 | 4.8 | ... | ... | ... | ... | N | |||||
−0.7 ± 0.1 | 4.8 | ... | ... | ... | ... | |||||||
−0.3 ± 0.1 | 4.4 | ... | ... | ... | ... | |||||||
RX J0506.8−0327 | −6.0 ± 0.2 | 6.1 | ... | ... | ... | ... | N | |||||
−5.8 ± 0.1 | 6.1 | ... | ... | ... | ... | |||||||
RX J0506.8−0305 | −4.7 ± 0.1 | 5.8 | −0.25 ± 0.01 | 4.3 | ... | ... | N | |||||
TTS J050649.8−031933 | −15.5 ± 1.00 | 6.5 | Y | G | ||||||||
TTS J050649.8−032104 | −65.7 ± 0.6 | 7.4 | −0.98 ± 0.06 | 5.3 | ... | ... | Y | |||||
−25.4 ± 0.3 | 7.0 | ... | ... | ... | ... | |||||||
TTS J 050650.5−032014 | −14.00 ± 1.00 | 6.1 | N | G | ||||||||
TTS J050650.7−032008 | −26.00 ± 0.50 | 6.6 | Y | G | ||||||||
RX J0506.9−0319 NW | −1.5 ± 0.1 | 5.7 | ... | ... | ... | ... | N | |||||
RX J0506.9−0319 SE | −4.1 ± 0.2 | 6.9 | ... | ... | ... | ... | Y | |||||
−4.2 ± 0.1 | 6.9 | ... | ... | ... | ... | |||||||
RX J0506.9−0320 W | −2.1 ± 0.1 | 6.4 | ... | ... | ... | ... | N | |||||
RX J0506.9−0320 E | −1.4 ± 0.1 | 6.8 | ... | ... | ... | ... | N | a | ||||
−1.6 ± 0.1 | 6.9 | ... | ... | ... | ... | |||||||
−1.6 ± 0.1 | 6.9 | ... | ... | ... | ... | |||||||
−1.8 ± 0.1 | 6.9 | ... | ... | ... | ... | |||||||
TTS J050654.5−032046 | −60.00 ± 5.00 | 7.3 | Y | G | ||||||||
LkHα 333 | −48.0 ± 0.8 | 8.1 | −0.08 ± 0.01 | 5.4 | −0.14 ± 0.01 | 5.6 | Y | |||||
−47.2 ± 3.4 | 8.1 | −8.6 ± 0.2 | 7.4 | −0.37 ± 0.01 | 6.1 | −0.02 ± 0.01 | 4.8 | |||||
... | ... | −8.9 ± 0.3 | 7.5 | ... | ... | ... | ... | |||||
−53.4 ± 1.4 | 8.2 | −8.8 ± 0.2 | 7.5 | −0.51 ± 0.01 | 6.2 | −0.04 ± 0.01 | 5.0 | |||||
−55.2 ± 1.8 | 8.2 | −9.5 ± 0.1 | 7.5 | −0.71 ± 0.02 | 6.4 | −0.10 ± 0.01 | 5.4 | |||||
−51.9 ± 1.6 | 8.2 | −9.1 ± 0.5 | 7.5 | −0.55 ± 0.01 | 6.2 | −0.08 ± 0.01 | 5.4 | |||||
−57.9 ± 0.2 | 8.2 | −9.6 ± 0.3 | 7.5 | −0.62 ± 0.01 | 6.3 | −0.11 ± 0.01 | 5.5 | |||||
L1616 MIR 4 | −28.6 ± 0.3 | 8.1 | ... | ... | ... | ... | Y | |||||
−25.2 ± 0.6 | 8.0 | ... | ... | ... | ... | |||||||
−26.5 ± 0.3 | 8.0 | ... | ... | ... | ... | |||||||
−26.0 ± 0.8 | 8.0 | ... | ... | ... | ... | |||||||
RX J0507.0−0318 | −1.3 ± 0.1 | 5.9 | ... | ... | ... | ... | N | |||||
−1.0 ± 0.1 | 5.8 | ... | ... | ... | ... | |||||||
−1.4 ± 0.1 | 6.0 | ... | ... | ... | ... | |||||||
TTS J050657.0−031640 | −94.00 ± 2.00 | 7.2 | Y | G | ||||||||
TTS J050704.7−030241 | −17.50 ± 1.00 | 6.3 | N | G | ||||||||
TTS J050705.3−030006 | −2.00 ± 0.40 | 6.2 | N | G | ||||||||
RX J0507.1−0321 | −37.1 ± 0.9 | 7.3 | −0.53 ± 0.01 | 5.2 | −0.37 ± 0.01 | 5.3 | Y | |||||
−36.9 ± 0.5 | 7.3 | −0.51 ± 0.01 | 5.2 | −0.40 ± 0.01 | 5.3 | |||||||
TTS J050706.2−031703 | −13.50 ± 0.50 | 6.1 | N | G | ||||||||
RX J0507.2−0323 | −1.2 ± 0.1 | 6.5 | ... | ... | ... | ... | N | |||||
TTS J050713.5−031722 | −10.50 ± 0.50 | 7.1 | N | G | ||||||||
RX J0507.3−0326 | −2.1 ± 0.1 | 6.1 | ... | ... | ... | ... | N | |||||
−1.8 ± 0.1 | 6.1 | ... | ... | ... | ... | |||||||
TTS J050717.9−032433 | −3.4 ± 0.1 | 6.1 | ... | ... | ... | ... | N | |||||
−4.0 ± 0.1 | 6.1 | −0.11 ± 0.01 | 4.4 | ... | ... | |||||||
RX J0507.4−0320 | −4.3 ± 0.1 | 5.8 | −0.16 ± 0.02 | 4.2 | ... | ... | N | |||||
−3.8 ± 0.1 | 5.8 | −0.08 ± 0.01 | 3.9 | ... | ... | |||||||
−3.9 ± 0.1 | 5.8 | −0.09 ± 0.01 | 3.9 | ... | ... | |||||||
RX J0507.4−0317 | −2.7 ± 0.1 | 6.0 | ... | ... | ... | ... | N | |||||
−6.0 ± 0.1 | 6.3 | −0.09 ± 0.01 | 4.3 | ... | ... | |||||||
−5.7 ± 0.1 | 6.3 | −0.16 ± 0.01 | 4.5 | ... | ... | |||||||
TTS J050729.8−031705 | −4.8 ± 0.1 | 5.6 | ... | ... | ... | ... | N | |||||
−0.8 ± 0.1 | 4.9 | ... | ... | ... | ... | |||||||
−9.2 ± 0.2 | 5.9 | ... | ... | ... | ... | |||||||
TTS J050730.9−031846 | −52.0 ± 1.4 | 6.9 | ... | ... | ... | ... | Y | |||||
−69.3 ± 2.6 | 7.1 | ... | ... | ... | ... | |||||||
TTS J050733.6−032517 | −2.30 ± 0.20 | 5.5 | N | G | ||||||||
TTS J050734.8−031521 | −1.6 ± 0.1 | 5.5 | ... | ... | ... | ... | N | |||||
−2.7 ± 0.1 | 5.7 | ... | ... | ... | ... | |||||||
−4.6 ± 0.1 | 5.9 | −2.24 ± 0.07 | 5.4 | ... | ... | b | ||||||
RX J0507.6−0318 | −1.2 ± 0.1 | 6.1 | ... | ... | ... | ... | N | |||||
−1.6 ± 0.1 | 6.2 | ... | ... | ... | ... | |||||||
−1.6 ± 0.1 | 6.2 | ... | ... | ... | ... | |||||||
TTS J050741.0−032253 | −4.30 ± 0.10 | 5.9 | N | G | ||||||||
TTS J050741.4−031507 | −6.80 ± 0.40 | 6.1 | N | G | ||||||||
TTS J050752.0−032003 | −9.50 ± 0.20 | 6.1 | N | G | ||||||||
TTS J050801.4−032255 | −21.50 ± 0.50 | 7.2 | Y | G | ||||||||
TTS J050801.9−031732 | −15.50 ± 0.50 | 6.9 | Y | G | ||||||||
TTS J050804.0−034052 | −2.20 ± 0.20 | 5.9 | N | G | ||||||||
TTS J050836.6−030341 | −68.50 ± 1.00 | 7.4 | Y | G | ||||||||
TTS J050845.1−031653 | −6.70 ± 1.00 | 6.1 | N | G | ||||||||
RX J0509.0−0315 | 1.10 ± 0.20 | ... | N | G | ||||||||
RX J0510.1−0427 | −0.20 ± 0.20 | 5.8 | N | G | ||||||||
1RXS J051011.5−025355 | −0.10 ± 0.20 | 5.7 | N | G | ||||||||
RX J0510.3−0330 | 1.50 ± 0.20 | ... | N | G | ||||||||
1RXS J051043.2−031627 | 2.40 ± 0.20 | ... | N | G | ||||||||
RX J0511.7−0348 | 1.80 ± 0.20 | ... | N | G | ||||||||
RX J0512.3−0255 | −6.50 ± 0.50 | 7.4 | Y | G |
Notes. The columns list: star name (Col. 1); equivalent widths and observed fluxes of the Hα, Hβ, He i λ5876 Å, λ6678 Å, and λ7065 Å lines (Cols. 2−11); our classification as accretor or not (Col. 12); some notes (G: EWHα measured by Gandolfi et al. 2008; a: the EWHα refers to the emission in the central reversal; b: the helium emission is probably due to flare presence).
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