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Table 1

Molecular column densities derived toward the dust peaks of L1521E and L1544.

Molecule Column density (cm−2)

L1521E L1544
SO (1.6 ± 0.5) × 1013 (1.5 ± 0.5) × 1013
13CS (1.6 ± 0.5) × 1012 (2.5 ± 0.8) × 1011
OCS (2.3 ± 0.7) × 1013 (8.9 ± 2.7) × 1012
C2S (1.4 ± 0.4) × 1013 (4.8 ± 1.4) × 1012
C3S (8.2 ± 2.5) × 1013 (5.7 ± 1.7) × 1012
C33S (1.4 ± 0.4) × 1012 (2.3 ± 0.7) × 1011
C34S (2.9 ± 0.9) × 1012 (6.1 ± 1.8) × 1011
CC34S (8.3 ± 2.5) × 1011
HCS+ (1.1 ± 0.3) × 1012 (4.4 ± 1.3) × 1011
H2CS (1.8 ± 0.5) × 1013 (6.0 ± 1.8) × 1012
C17O (1.2 ± 0.4) × 1014
HC3N (8.4 ± 2.5) × 1012 (1.1 ± 0.3) × 1013
c-C3H2 (1.3 ± 0.4) × 1012 (4.3 ± 1.3) × 1012
C4H (1.6 ± 0.5) × 1014 (2.0 ± 0.6) × 1014
HN13C (6.0 ± 1.8) × 1011 (2.0 ± 0.6) × 1012
CH3OH (E2) (1.9 ± 0.6) × 1013 (2.2 ± 0.7) × 1013
CH3OH (A+) (5.7 ± 1.7) × 1012 (7.3 ± 2.2) × 1012
CH3CCH (2.1 ± 0.6) × 1013 (4.9 ± 1.5) × 1013
CH3CHO (8.3 ± 2.5) × 1010 (6.2 ± 1.9) × 1010
l-C4H2 (4.1 ± 1.2) × 1011
H2CCO (1.4 ± 0.4) × 1012
CH3CN (4.8 ± 1.4) × 1011 (6.1 ± 1.8) × 1011
HC18O+ (6.7 ± 2.0) × 1010 (8.3 ± 2.5) × 1010
H13CN (1.6 ± 0.5) × 1012 (2.6 ± 0.8) × 1012
HCO (7.0 ± 2.1) × 1011 (5.0 ± 1.5) × 1011
HCN (2.4 ± 0.7) × 1012 (1.3 ± 0.4) × 1012
HCO+ (1.3 ± 0.4) × 1012 (3.2 ± 1.0) × 1011
N2H+ (2.5 ± 0.8) × 1013 (2.0 ± 0.6) × 1014
HNCO (9.3 ± 2.8) × 1012 (1.6 ± 0.5) × 1013
C2H (7.6 ± 2.3) × 1013 (9.5 ± 2.9) × 1013
CN (1.2 ± 0.4) × 1013

Notes. The column densities toward L1544 are based on data from the ASAI (Lefloch et al. 2018). The assumed excitation temperature was 10 K for CO and 4.5 K for the other species for L1521E, and 5 K for L1544. The used transitions are shown in Table A.1 with asterisk, except for C3S (92488.5 MHz), CH3CHO (95947.4 MHz), and H2CCO (101981.4 MHz), to be consistent between the two sources. The SO column density is based on the 34SO column density and an isotopic ratio of 22 (Wilson & Rood 1994).

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