Pre-main-sequence star candidates in the bar of the large magellanic cloud

Science

Volumn 272, Issue 5264, 1996, Pages 995-997

  Beaulieu, J P ^a   Lamers, H J G L M ^a   Grison, P ^a   Julien, R ^a   Lanciaux, C ^a   Ferlet, R ^a   Vidal Madjar, A ^a   Bertin, E ^a   Maurice, E ^a   Prevot L ^a   Gry, C ^a   Guibert, J ^a   Moreau, O ^a   Tajhmady, F ^a   Aubourg, E ^a   Bareyre, P ^a   De Kat, J ^a   Gros, M ^a   Laurent, B ^a   Lachieze Rey M ^a   Lesquoy, E ^a   Magneville, C ^a   Milsztajn, A ^a   Moscoso, L ^a   Queinnec, F ^a   Renault, C ^a   Rich, J ^a   Spiro, M ^a   Vigroux, L ^a   Zylberajch, S ^a   Ansari, R ^a   Cavalier, F ^a   Moniez, M ^a   more..

^a NONE

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; ASTRONOMY; CLOUD; PHOTOMETRY; PRIORITY JOURNAL;

EID: 0141742836     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.272.5264.995     Document Type: Article

References (13)

1. C) [P. Grison et al., Astron. Astrophys. Suppl. Ser. 109, 447 (1995)]. An astrometric calibration gave coordinates accurate to ∼3 arc sec.
2. C) [P. Grison et al., Astron. Astrophys. Suppl. Ser. 109, 447 (1995)]. An astrometric calibration gave coordinates accurate to ∼3 arc sec.
3. C) [P. Grison et al., Astron. Astrophys. Suppl. Ser. 109, 447 (1995)]. An astrometric calibration gave coordinates accurate to ∼3 arc sec.
4. C) [P. Grison et al., Astron. Astrophys. Suppl. Ser. 109, 447 (1995)]. An astrometric calibration gave coordinates accurate to ∼3 arc sec.
5. C) [P. Grison et al., Astron. Astrophys. Suppl. Ser. 109, 447 (1995)]. An astrometric calibration gave coordinates accurate to ∼3 arc sec.
6. Th. Schmidt-Kaler, Landolt-Bornstein, vol. 2, Astronomy and Astrophysics Subvolume B, K. Schaifers and H. H. Voigt, Eds. (Springer-Verlag, Berlin, 1982), pp. 18-20.
7. P. S. Thé, in The Nature and Evolutionary Status of Herbig Ae/Be Stars (ASP Conference Series, vol. 62), P. S. Thé and M. R. Perez, Eds. (Astronomical Society of the Pacific, San Francisco, 1994), pp. 23-29.
8. -1. The flux calibration has a precision of ∼5% near Hα and ∼10% near 4000 Å. The signal/noise ratio of the spectra is between 15 (for ELHC7) and 75 (for ELHC5 and ELHC6).
9. G. Ortiz et al., in (3), pp. 128-129.
10. T. Bohm and C. Catala, Astron. Astrophys. Suppl. Ser. 101, 629 (1993) presented arguments that for some galactic HAeBe stars, the excess Balmer continuum is attributable to the stellar wind rather than to an accretion disk.
11. F. Palla and S. W. Stahler, Astrophys. J. 418, 414 (1993); in (3), pp. 391-403.
12. F. Berrilli et al., Astrophys. J. 398, 254 (1992).
13. This work is based on observations made at ESO La Silla, We thank A. Smette for kindly giving up some of his observing time.