Upper limits to the detection of ammonia from protoplanetary disks around HL Tauri and L1551-IRS 5

Details Upper limits to the detection of ammonia from protoplanetary disks around HL Tauri and L1551-IRS 5 Upper limits to the detection of ammonia from protoplanetary disks around HL Tauri and L1551-IRS 5

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...414..333g&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 414, no. 1, p. 333-336.

Astronomy and Astrophysics

Astrophysics

6

Ammonia, Early Stars, Pre-Main Sequence Stars, Protoplanets, Stellar Envelopes, Taurus Constellation, Angular Resolution, Planetary Systems, Very Large Array (Vla)

Scientific paper

We present NH3(1, 1) and (2, 2) observations of the young stellar sources HL Tau and L1551-IRS 5 using the VLA in its B-configuration, which provides an angular resolution of about 0.4 arcsec (about 50 AU at 140 pc) at 1.3 cm wavelength. Our goal was to detect and resolve circumstellar molecular disks with radius of the order of 100 AU around these two sources. No ammonia emission was detected toward either of them. The 3-sigma levels were 2.7 mJy/beam and 3.9 mJy/beam for HL Tau and L1551-IRS 5, respectively, with a velocity resolution of about 5 km/s. With this nondetection, we estimate upper limits to the mass of the proposed protoplanetary molecular disks (within a radius of 10 AU from the central stars) on the order of 0.02/(X(NH3)/10 exp -8) solar mass for HL Tau and 0.1/(X(NH3)/10 exp -8) solar mass for L1551-IRS 5.

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