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HD 35408


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Oscillations in the PMS delta Scuti star V346 Ori
We report the discovery of periodicities in the light curve of thePre-Main Sequence (PMS) Herbig Ae star V346 Ori. We interpret variationsin the light curve of the star as the superposition of at least twoperiodic signals that result from delta Scuti-type stellaroscillations. The computation of linear non-adiabatic radial pulsationmodels for PMS stars reproduces these periods for a 1.55 Msunstar with Teff = 7410 K and log L/Lsun = 0.74pulsating in the fundamental and in the second overtone. If ourassumption of radial oscillations is indeed correct, the star's locationon the HR diagram places it at a distance significantly smaller thanthat of the Orion star forming region, hence raising questions regardingthe evolutionary status of V346 Ori. Observations with better timesampling and spanning a longer period of time are needed if the latterquestion is to be addressed fully.Tables 1 and 2 are only available in electronic form at the CDS viaanonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/399/271

Walraven photometry of nearby southern OB associations
Homogeneous Walraven (VBLUW) photometry is presented for 5260 stars inthe regions of five nearby southern OB associations: Scorpio Centaurus(Sco OB2), Orion OB1, Canis Major OB1, Monoceros OB1, and Scutum OB2.Derived V and (B - V) in the Johnson system are included.

The Meridian Proper Motions of 161 Stars in the Region of the Belt of Orion.
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Datos observacionales y astrométricos

Constelación:Orión
Ascensión Recta:05h24m36.62s
Declinación:+01°48'03.5"
Magnitud Aparente:8.94
Movimiento Propio en Ascensión Recta:0
Movimiento Propio en Declinación:0.3
B-T magnitude:8.988
V-T magnitude:8.944

Catálogos y designaciones:
Nombres Propios
HD 1989HD 35408
TYCHO-2 2000TYC 101-205-1
USNO-A2.0USNO-A2 0900-01612406

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