III/267 Spectral types from Uppsala Observatory (Schalen, 1948-1949)
Spectra, magnitudes, and colours of stars in regions of different galactic
latitude (parts I and II)
Schalen C.
<Uppsala Astron. Obs. Ann. 2, part 4 (1948); 3, part 3 (1949)>
=1948UppAn...2d....S 1948UppAn...2d....S
=1949UppAn...3c....S 1949UppAn...3c....S
=2013yCat.3267....0S 2013yCat.3267....0S
ADC_Keywords: Spectral types
Description:
The two papers compiled here contain spectral types for about 2600
stars in two regions near +20 deg and +40 deg galactic latitude at
far-northern Declination. The +20 deg latitude region extends from
about RA 19h30m to 0h00m; the +40 deg latitude region extends from
about RA 10h to 15h45m. Each zone is about 5 deg in width and the
faintest stars are about V mag 11. This includes nearly all BD stars
plus many fainter ones. A statistical study of these stars was
presented in a third paper (1954ArA.....1..483S 1954ArA.....1..483S).
The source material consists of objective-prism plates taken between
1934 and 1940 with the Zeiss-Heyde astrograph (15cm aperture f/10
triplet) of the Uppsala Observatory. The 9.7-deg prism gave a
dispersion of 1.4mm between H-gamma and H-epsilon, roughly 260A/mm.
The stars were classified on the basis of microphotometer tracings of
the spectra.
For the present list only the spectral types have been preserved,
and various magnitudes, line-ratios, and color-equivalents omitted.
The coordinates are mainly from Tycho-2. The magnitudes close to
standard V are from modern sources including Tycho-2 and the TASS MkIV
survey. The Uppsala spectral types are expressed in MK notation,
specifically relating to dwarf/giant discrimination via the CN bands
for G and K stars, and some luminosity classification via Balmer
line-widths for stars between late-B and early-A. In principle, the
temperature types are matched to the HD scale.
A few "new" metallic-line A-type stars are reported here as well.
In addition, two mag 10 stars were identified by Schalen as type 'B'.
Examination of Burrell Schmidt objective-prism plates (uv-transparent
10-degree prism, 110A/mm) shows that both are previously unrecognized
B subdwarfs (BD+74 435 and BD+77 564 in the latitude +40 zone).
The catalogue contains many stars not classified, for instance,
in the HD or for the Yale and AGK astrometric catalogues. Similarly,
large numbers of BD stars without accurate coordinates are identified
here for the first time. Non-BD stars are assigned the acronyms [S48]
and [S49].
There are several clerical errors in the published tables such that
stars are either not the named BD star or are not recovered near the
nominal coordinates. A combination of the spectral types and more
recent photometric colors was used to identify candidates within about
10' radius, but a few stars remain lost.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
stars.dat 114 2606 Spectral classifications of the stars studied.
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Byte-by-byte Description of file: stars.dat
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Bytes Format Units Label Explanations
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1- 5 A5 --- Cat Desgination of Catalog (BD, [S48] or [s49]) (1)
7- 10 I4 --- Seq Sequentiel number in zone or part (1)
18- 19 I2 h RAh Right Ascension J2000 (hours) (2)
21- 22 I2 min RAm Right Ascension J2000 (minutes) (2)
24- 28 F5.2 s RAs Right Ascension J2000 (seconds) (2)
30 A1 --- DE- Declination J2000 (sign) (2)
31- 32 I2 deg DEd Declination J2000 (degrees) (2)
34- 35 I2 arcmin DEm Declination J2000 (minutes) (2)
37- 40 F4.1 arcsec DEs ?Declination J2000 (seconds) (2)
42 A1 --- s [TUM*] Source of position (2)
44- 47 F4.1 mag mag ? Apparent magnitude (from B. Skiff)
49 A1 --- n_mag [V*] Magnitude band (* for stars not found)
52- 61 A10 --- SpType MK spectral type
62-114 A53 --- Comments Notes and comments (from B. Skiff)
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Note (1): the name is:
* for Part.I of both papers: the BD number (Cat. I/122)
Note that wrong BD numbers are written "**", a corrected
identification of the star is given in the notes (a TYC number)
* for Part.II of Paper I (1948): [S48] followed by the running number
* for Part.II of Paper II (1949): [S49] followed by the running number
Note (2): for stars not found, the position is the one given in the catalog
and precessed to J2000 -- the fractions of seconds and arcseconds are
blanked, and the source is marked with an asterisk (*). The codes are:
M = 2MASS (II/246)
U = UCAC4 (I/322)
T = Tycho-2 (I/259)
* = stars not found (4 stars: one for [S48] and 3 for [S49])
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History:
Prepared by B. Skiff [Lowell Obs.]
(End) B. Skiff [Lowell Obs.], Francois Ochsenbein [CDS] 13-Jan-2013