SpectraDB

WR 1

Observer: GDAA

Spectrum Data

FITS Header Metadata

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Key Value
SIMPLE True
BITPIX -32
NAXIS 1
NAXIS1 2774
CRPIX1 1
CDELT1 1.44384545519857
CRVAL1 3797.88159179688
CTYPE1 Wavelength
CUNIT1 Angstrom
SWCREATE RSpec 2.1.1.18
VERSION RSpec 2.1.1.18
OBSERVER HLAD
BSS_SITE Sandvreten Observatory L11
BSS_INST T41
OBJNAME WR 1
DATE-OBS 2025-12-20T20:38:33
EXPTIME 1800
BSS_VHEL 0

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Calibrated Spectrum

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Observation Image

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Metadata

FieldValue
Object NameWR 1
ObserverGDAA
Site Sandvreten Observatory
EquipmentT41
Observation Date2026-01-25 11:36
Julian Date2461065.98333
Created2026-01-25 11:36
Updated2026-02-11 16:09

Notes

From Wikipedia: WR 1 is a Wolf-Rayet star located around 10,300 light years away from Earth in the constellation of Cassiopeia. It is only slightly more than twice the size of the sun, but due to a temperature over 100,000 K it is over 758,000 times as luminous as the sun. Although WR 1 has been recognised as a Wolf-Rayet star since the 19th century,[9] the WR 1 designation does not indicate that it was the first to be discovered. Ordered by right ascension, WR 1 is the first star in the Seventh Catalogue of galactic Wolf-Rayet stars.[10] WR 1 is a member of the nitrogen sequence of WR stars and has a spectrum with HeII lines much stronger than HeI lines, and NV emission more than twice the strength of NIII, leading to the assignment of a WN4 spectral type. The spectrum has particularly wide HeII, leading to the equivalent classifications of WN4-b (for broad) or WN4-s (for strong). The spectrum also includes CIV and NIV, but no hydrogen lines at all indicating that WR 1 has already expelled all of its hydrogen through its powerful solar winds

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