Open Access

Table 1.

Evolutionary stages of DPV V4142 Sgr.

Stage Age (Myr) M (M) R (R) Po (d) Log T (K) (M yr−1) Ev. process
Donor A 0.000 3.5000 2.2246 15.0000 4.1325 −3.9127E−12 Zero Age Main Sequence (ZAMS)
B 0.8910 3.4997 2.6004 15.0027 4.1130 −3.6946E−12 Terminal Age Main Sequences (TAMS)
X1 138.0000 3.4995 2.9399 15.0045 4.1010 −4.9005E−12 Inversion of the 1H/4He ratio
C 278.5000 3.4930 7.2768 15.0456 3.9665 −2.2170E−10 Depletion of central hydrogen 1H
D 279.7160 3.4927 6.1764 15.0471 4.0229 −1.3642E−10 Size increase beyond the RL due to depletion of 1H
E 280.0550 3.4863 19.8061 14.9438 3.7316 −3.7128E−06 Initiation of mass transfer
U1 280.1115 2.4907 11.8353 8.9929 3.6434 −2.2477E−05 Mass inversion
F 280.1337 1.9019 11.8784 10.7057 3.6265 −2.9974E−05 Minimum Roche lobe value
G 280.1578 1.1747 17.0432 24.0015 3.6119 −2.1044E−05 End of optically thick mass transfer (U2)
X2 280.1676 1.0477 19.2030 30.6325 3.6463 −7.7595E−06 Current stage
H 280.9710 0.7026 30.2055 77.1262 3.7964 −2.8307E−08 End mass transfer stage
I 306.0468 0.6883 0.2368 7.5859 4.5723 −3.7117E−10 Helium depletion (4He)

Gainer
a 0.000 1.5000 1.4857 15.000 3.8444 −2.0314E−12 Zero Age Main Sequence (ZAMS)
b 280.0550 1.5057 1.8255 14.9438 4.0391 3.6931E−06 Initiation of mass accretion
c 280.0900 2.0795 16.6218 9.7658 3.8433 2.0099E−05 Rejuvenation by hydrogen 1H
U1 280.1115 2.4962 18.7188 8.9929 3.8588 2.2360E−05 Mass inversion
d 280.1337 3.0818 18.0276 10.7057 3.9272 2.9817E−05 Return to the Main Sequence (RMS)
e 280.1578 3.8052 10.4409 24.0015 4.0842 2.0936E−05 Transition to the threshold of rejuvenated B type stars
X2 280.1676 3.9316 6.3856 30.6325 4.1702 7.7184E−06 Current stage
f 280.9710 4.2672 2.2439 77.1262 4.2185 4.8843E-09 End of mass accretion and relocation to the MS
g 306.0468 4.2668 2.6559 7.5859 4.1957 −2.0541E−11 Second Main Sequence turnoff

Notes. Exploring the evolutionary stages of DPV V4142 Sgr: from the ZAMS to 4He depletion of the donor star. Detailed descriptions of key features are provided, along with corresponding ages measured in Mega years (Myr). Additionally, the threshold of rejuvenation for B-type stars is presented.

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