1991ApJ...382..270W


Query : 1991ApJ...382..270W

1991ApJ...382..270W - Astrophys. J., 382, 270-289 (1991/November-3)

Are FU Orionis stars younger than T Tauri stars ? Submillimeter constraints on circumstellar disks.

WEINTRAUB D.A., SANDELL G. and DUNCAN W.D.

Abstract (from CDS):


Abstract Copyright: ∼

Journal keyword(s): Stars: Circumstellar Shells - Stars: Pre-Main-Sequence - Stars: Radio Radiation

Simbad objects: 8

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Number of rows : 8
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 V* FU Ori Or* 05 45 22.3647842544 +09 04 12.291320064   10.72 9.60     F0Iab 888 1
2 V* Z CMa Ae* 07 03 43.1599411656 -11 33 06.209065836 10.51 9.99 8.80     B5/8eq+F5/7 601 3
3 V* V646 Pup Or* 07 50 35.5923145848 -33 06 23.905800180   13.96 12.65 12.04   ~ 77 0
4 IRAS 16289-4449 Or* 16 32 32.19264 -44 55 30.6552       15.95   ~ 149 1
5 V* V1515 Cyg Or* 20 23 48.0158573016 +42 12 25.781279076   15.26 13.39 12.03   G0/G2Ib 260 0
6 EM* LkHA 190 Or* 20 58 53.7335347296 +44 15 28.388727720   14.26 12.33 12.13   F7/G3I/IIe 530 0
7 EM* LkHA 120 Or* 21 01 09.2070147480 +50 21 44.806779000 13.37 13.09 11.99 11.75   F0/F4-G5 203 1
8 V* V1735 Cyg Or* 21 47 20.6628414360 +47 32 03.857457372           ~ 170 0

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