J21255-5459

Culpan hotsd

χ²/N = 0.99

Spectrum

shaded: the intervals the fit used ·  │ a cancelled pixeldrag on either panel to zoom · dbl-click or Esc to reset · arrows to pan

The whole reduced spectrum above, the region marked on it below. Shaded bands are the intervals the fit used; a tick under the axis marks a pixel the rejection mask cancelled.

Line-profile fit — Bamberg

profile fit on the Bamberg grid
Observed spectrum in black, model in red, offset by line. Balmer series left, helium right.

Results and provenance

Fit — Bamberg

Teff [K]48656 ± 1590
log g6.241 ± 0.148
log n(He)/n(H)-1.796 ± 0.150
reduced χ²0.986 over 746 points
radial velocity-108.0 km s−1
resolution (FWHM)2.00 Å
lines fitted15
gridsHE-0.041.fits
HE-0.125.fits
HE-0.300.fits
HE-0.550.fits
+9 more
fitted04/09/2026 19:10:41

Observation

source filespec-106209-60208-63050396475010092.fits

Gaia astrometry

Gaia DR3 source6463280508889841408
parallax [mas]0.3870 ± 0.0609
G16.798
BP − RP-0.457
Gabs4.736
μα [mas/yr]0.381
μδ [mas/yr]-2.859
RUWE0.994
l, b341.336, -43.749
selectionf_plx

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-1.75-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.56-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.48-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.43-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.40-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.38-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.37-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.36-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-1.69-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-1.95-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-1.64-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-1.51-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-1.61-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.45-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-1.77-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 48656 K · log g 6.241 · E(44−55) 0.030 · χ²r 0.21 over 34 bands

distance 2584 pc · parallax 0.3900 ± 0.0600 mas (15%) · R 0.1015 +0.0191 −0.0138 R☉ · M 0.657 +0.290 −0.179 M☉ — above the 0.47 canonical mass · L 52.1 +21.4 −13.3 L☉

Photometry against the model, with the residual beneath it in units of the error. The horizontal bar on each point is the passband, not an error; a hollow point was not fitted and the tooltip says why. Drag a box to zoom, double-click or Esc to come back out.