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 |
FITS Spectral Image
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Calibrated Spectrum
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Metadata
| Field | Value |
|---|---|
| Object Name | WR 1 |
| Observer | GDAA |
| Site | Sandvreten Observatory |
| Equipment | T41 |
| Observation Date | 2026-01-25 11:36 |
| Julian Date | 2461065.98333 |
| Created | 2026-01-25 11:36 |
| Updated | 2026-02-11 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