SIMBAD references

1999ApJ...517..256K - Astrophys. J., 517, 256-263 (1999/May-3)

Near-infrared spectropolarimetry of three prototype low-mass young stellar objects in the Taurus dark cloud.


Abstract (from CDS):

We present near-infrared spectropolarimetric data between 0.9 and 4.2 µm for three prototypes of low-mass young stellar objects (YSOs), L1551 IRS 5, HL Tau, and T Tau in the Taurus dark cloud. These sources are in different classes in the standard spectral classification scheme of low-mass YSOs by Lada. The polarization curves of the observed sources show distinct differences. The class I protostar L1551 IRS 5 shows a flat polarization curve with high polarization through the observed wavelengths. It also shows a polarization excess at the 3.1 µm ice band absorption feature. The ``flat-spectrum source'' HL Tau, which is thought to be in a transient phase from class I to class II, shows a steep decrease of polarization with increasing wavelengths from 1.0 to 2.5 µm, while it shows a flat polarization curve with high polarization in optical wavelengths and a slowly decreasing slope with small polarization in 3-4 µm. The class II source T Tau displays small polarization no more than 2% through the observed wavelengths; the polarization in the shorter wavelengths from optical to 1.3 µm decreases with increasing wavelengths. T Tau also shows an increasing polarization curve in the longer wavelengths over 1.6 µm, which is most likely to come from the infrared companion T Tau S (Kobayashi et al.). The prominent differences of the observed near-infrared polarization curves can be clearly understood in terms of the standard spectral classification scheme of low-mass YSOs. Thus near-infrared spectropolarimetry could serve as a potentially powerful diagnostic of circumstellar material, complementary to the standard spectral classification.

Abstract Copyright:

Journal keyword(s): ISM: Dust, Extinction - ISM: Jets and Outflows - Polarization - Scattering - Stars: Formation - Stars: Pre-Main-Sequence

Simbad objects: 11

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