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MICHIGAN: Two-dimensional spectral types for HD stars(IV)
Contents
Table name: Michigan
Records: 33301
Spectral Band: OPT,Photo
Kind of Object: HD-Star
Mode: Spectroscopy,Objective-Prism
PreView:
Coordinates: J2000
Reference
- Michigan Catalogue of Two Dimensional Spectral Types for the HD,
Vol.4, Ann Arbor, Dept. of Astronomy, Univ. of Michigan
Description
This catalogue is part of a program of systematic reclassification of the
Henry Draper stars on the MK system and contains all HD stars between dec =
-26.0 and -12.0 degrees. The stars were classified visualy on
objective-prism plates taken with the Michigan Curtis Schmidt telescope at
Cerro Tololo Inter-American Observatory. The 4 + 6 degrees prisms yield a
dispersion at Hgamma of 108 Angstrom/mm, and the resolution is about 2
Angstrom/mm, comparable to that of the original MK system. The spectra were
taken on IIaO plates and widened to 0.8 mm, with 20 min, 4min, 1min
exposures being obtained. The high quality of the spectra is illustrated in
'An Atlas of Objective-Prism Spectra' by N.Houk, N.J. Irvine and D.
Rosenbush and 'A Second Atlas of Objective-Prism Spectra' by Nancy Houk and
Michael V. Newberry. In order to mantain a uniform, consistent system, all
the spectra classification was done by one person(NH). Over 170 standard
stars were used. Of the 33301 stars in the catalogue, 32563 (98%) were
classifiable. Internal classification errors were obtained using the stars
classified independently on more than one plate. Both internal and external
errors are similar to those usually obtained in the classification of slit
spectra. 15% of the stars have remarks giving futher information. (See also
the R_MICHIGAN catalogue.)
Fields
Name Meaning
HD HD number
pmag Photographic magnitude
pecul Flag about peculiarity
sp Spectral type
others + means that the sp is taken from another source
qur Quality and Remarks code
Quality: 1 (best) to 4 (worst)
Remarks code: B,L,O,R,D
var V means that the star is variable
remark Remark from the r_michigan catalogue
ra_ori Right ascension: epoch 1900.0
dec_ori Declination: epoch 1900.0
lii_ori Galactic longitude (integer 2 bytes)
bii_ori Galactic latitude (integer 2 bytes)
ra Right ascension: epoch 2000.0
dec Declination: epoch 2000.0
lii Galactic longitude (integer 4 bytes)
bii Galactic latitude (integer 4 bytes)
prc_ra 100 years Precession in (alp)
prc_dec 100 years Precession in (del)
DM DM number
SAO SAO number
plate Plate codes
REMARKS
Further information about 5144 stars is given in the 'remark' field (taken
from the r_michigan catalogue). The kind of information that one can find in
this field is indicated in the 'qur' field:
- B Indicates that the remark contains the HR (Bright Star Catalogue)
number and the Bayer or Flamsteed designations where applicable (1154
stars).
- L Indicates that information from the astronomical literature is given.
Remarks were generally restricted to those relevant to the spectral
appearance, such as rotation, variability, and duplicity, and generally
have included only information about the star which might affect the
spectral classification.
The entry "emission catalogue" refers to Wackerling's catalogue.
- O Includes 355 remarks that do not fit into any other catalogue. Almost
all of these are NGC or IC designations for nebulae or identification
numbers from the CoD, SD, etc.
- R 1147 of the stars in the remarks section have remarks of this type. All
'R' remarks were written by NH in the course of the spectral
classification and are all related in some way to the spectrum.
- D The Stellar Data Center at Strasbourg provided a listing of visual
double stars. Remarks beginning "undetected visual double" were
included for doubles not discovered in the course of the spectral
classification, the others having 'R' remarks.
D remarks were included for the 1932 doubles having a separation = 30
arcsec and a (DEL)mag > 4.0 mag, since for these the spectral
appearance and hence the assigned spectral type might be affected.
Spectra classified as weak metal, Am, or Ap were re-examined by Houk to
be sure these characteristics were not due to the double.