J/ApJ/700/844         Rotation rates of very massive stars        (Penny+, 2009)
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A FUSE survey of the rotation rates of very massive stars in the Small and Large
Magellanic Clouds.
    Penny L.R., Gies D.R.
   <Astrophys. J., 700, 844-858 (2009)>
   =2009ApJ...700..844P
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ADC_Keywords: Magellanic Clouds ; Stars, OB ; Ultraviolet ; Stars, early-type
              Rotational velocities
Keywords: Magellanic Clouds - stars: early-type - stars: rotation -
          ultraviolet: stars

Abstract:
    We present projected rotational velocity values for 96 Galactic, 55
    SMC, and 106 LMC O-B type stars from archival FUSE observations. The
    evolved and unevolved samples from each environment are compared
    through the Kolmogorov-Smirnov test to determine if the distribution
    of equatorial rotational velocities is metallicity dependent for these
    massive objects. Stellar interior models predict that massive stars
    with SMC metallicity will have significantly reduced angular momentum
    loss on the main sequence compared to their Galactic counterparts. Our
    results find some support for this prediction but also show that even
    at Galactic metallicity, evolved and unevolved massive stars have
    fairly similar fractions of stars with large Vsin i values.
    Macroturbulent broadening that is present in the spectral features of
    Galactic evolved massive stars is lower in the LMC and SMC samples.
    This suggests the processes that lead to macroturbulence are dependent
    upon metallicity.

Description:
    We obtained Far Ultraviolet Spectrographic Explorer (FUSE) archival
    spectra of 96 Galactic, 55 SMC, and 106 LMC massive stars that are
    available from the Multimission Archive at Space Telescope (MAST).

File Summary:
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 FileName   Lrecl  Records   Explanations
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ReadMe         80        .   This file
table1.dat     80       96  *Galactic targets
table2.dat    115       55   SMC targets
table3.dat    126      106   LMC targets
notes.dat      80       50   Individual note on objects
refs.dat       78       42   References
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Note on table1.dat: corrections made at CDS for 2 stars
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See also:
  II/236  : UBVR CCD survey of the Magellanic clouds (Massey+, 2002)
  III/147 : Studies of LMC stellar content (Rousseau+ 1978)
  J/PASP/121/634  : FUSE observations in Magellanic Clouds (Blair+, 2009)
  J/MNRAS/353/601 : 2dF survey of the Small Magellanic Cloud (Evans+, 2004)
  J/AJ/127/1632   : UBVR(UIT) photometry of O and OB stars in SMC (Oey+, 2004)
  J/ApJS/144/21   : Galaxy and Magellanic Clouds OB and WR stars (Robert+, 2003)
  J/MNRAS/324/33  : MC WC/WO stars - Colliding winds (Bartzakos+ 2001)
  J/AJ/121/891    : UBV photometry of LMC OB associations (Parker+, 2001)
  J/AJ/119/2214   : Photometry of Magellanic OB associations (Massey+, 2000)
  J/MNRAS/284/265 : Rotational Velocities of 373 OB stars (Howarth+ 1997)
  J/ApJS/91/583   : MC massive stars IMF. I. (Hill+, 1994)
  J/AJ/103/1205   : Stellar Content of LH 9 and 10 in the LMC (Parker+ 1992)
  http://archive.stsci.edu/fuse/ : MAST FUSE home page

Byte-by-byte Description of file: table1.dat
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   Bytes Format Units   Label     Explanations
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   1- 12  A12   ---     Name      Star name (BD names corrected at CDS)
  14- 27  A14   ---     SpT       MK spectral type from Howarth et al. 1997,
                                  Cat. J/MNRAS/284/265
  29- 31  I3    km/s    <vsini>H  Mean Vsini from Howarth et al. 1997,
                                  Cat. J/MNRAS/284/265
  33- 35  I3    km/s    <vsini>A  Mean Vsini computed from the calibration of
                                  AV 327 template star
  37- 39  I3    km/s    <vsini>S  ?=- Mean Vsini computed from the calibration
                                  of SK-66 100 template star
  41- 80  A40   ---     Set       FUSE observation(s) data set used
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Byte-by-byte Description of file: table[23].dat
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   Bytes Format Units  Label      Explanations
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   1- 13  A13   ---    Name       Star name
  15- 30  A16   ---    SpT        MK spectral type
  31- 32  I2    ---  r_SpT        ? Reference for spectral classification (1)
  34- 36  I3    km/s   <vsini>    Mean vsini from this paper
  38- 40  I3    km/s   <vsini>2   ? Second measure of <vsini>
  42- 44  I3    km/s   <vsini>L   ? Mean vsini from litterature
      45  A1    ---  r_<vsini>L   Reference for <vsini>L (1)
  47- 49  I3    km/s   <vsini>L2  ? Second mean vsini from litterature
      50  A1    ---  r_<vsini>L2  Reference for <vsini>L2 (1)
  52- 54  I3    km/s   <vsini>L3  ? Third mean vsini from litterature
      55  A1    ---  r_<vsini>L3  Reference for <vsini>L3 (1)
  57- 58  I2    km/s   <vsini>L4  ? Fourth mean vsini from litterature
      59  A1    ---  r_<vsini>L4  Reference for <vsini>L4 (1)
  61- 70  A10   ---    TStar      Template star name
  72-101  A30   ---    Set        FUSE data set(s)
 103-126  A24   ---    Note       Notes (*: note in notes.dat file) (2)
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Note (1): See refs.dat file
Note (2): Stars with a "NO" in this column are excluded from our analysis
     for various reasons.
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Byte-by-byte Description of file: notes.dat
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   Bytes Format Units   Label     Explanations
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   1- 13  A13   ---     Name      Star name
  15- 80  A66   ---     Note      Text of note
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Byte-by-byte Description of file: refs.dat
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   Bytes Format Units   Label     Explanations
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   1-  2  A2    ---     Ref       Reference number
   4- 22  A19   ---     BibCode   Bibcode
  24- 48  A25   ---     Aut       Author's name
  50- 78  A29   ---     Comm      Comment
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History:
    From electronic version of the journal

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(End)                                     Emmanuelle Perret [CDS]    21-Jul-2011
