Table 1
Main properties of our target, L1527 IRS.
| Alternative ID | IRAS 04368+2557 |
|---|---|
| RA | 04h 39m 53.88s |
| Dec | +26° 03′09″.56 |
| Age (yr) | <3 × 105[1] |
| M*(M⊙) | 0.2[1]−0.45[1,2] |
| Lbol(L⊙) | 1.6[3] |
 |
0.8[4] |
Notes. The age of the object has been roughly estimated by [1] (Tobin et al. 2012) based on the mass loss rate of the source. The mass of the protostar has been estimated by means of kinematical analysis by [1] and [2] (Aso et al. 2017). The bolometric luminosity was reported by [3] (Karska et al. 2018) and might suffer up to a factor two uncertainty due to the high inclination of the disk (e.g., Whitney et al. 2003). The envelope mass was derived in [4] (Motte & André 2001) based on the IRAM 30 m telescope and MPIfR bolometer arrays’ 1.3 millimeter maps.
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