TY - JOUR
T1 - Low- J Transitions in A 2 Π ( 0 , 0 , 0 ) - X 2 ς + ( 0 , 0 , 0 ) Band of Buffer-gas-cooled CaOH
AU - Takahashi, Yuiki
AU - Baba, Masaaki
AU - Enomoto, Katsunari
AU - Hiramoto, Ayami
AU - Iwakuni, Kana
AU - Kuma, Susumu
AU - Tobaru, Reo
AU - Miyamoto, Yuki
N1 - Publisher Copyright:
© 2022. The Author(s). Published by the American Astronomical Society.
PY - 2022/9/1
Y1 - 2022/9/1
N2 - Calcium monohydroxide radical (CaOH) is receiving an increasing amount of attention from the astrophysics community as it is expected to be present in the atmospheres of hot rocky super-Earth exoplanets as well as interstellar and circumstellar environments. Here, we report the high-resolution laboratory absorption spectroscopy on low-J transitions in A 2Π(0,0,0)-X 2ς+(0,0,0) band of buffer-gas-cooled CaOH. In total, 40 transitions out of the low-J states were assigned, including 27 transitions that have not been reported in previous literature. The determined rotational constants for both ground and excited states are in excellent agreement with previous literature, and the measurement uncertainty for the absolute transition frequencies was improved by more than a factor of 3. This will aid future interstellar, circumstellar, and atmospheric identifications of CaOH. The buffer-gas-cooling method employed here is a particularly powerful method to probe low-J transitions and is easily applicable to other astrophysical molecules.
AB - Calcium monohydroxide radical (CaOH) is receiving an increasing amount of attention from the astrophysics community as it is expected to be present in the atmospheres of hot rocky super-Earth exoplanets as well as interstellar and circumstellar environments. Here, we report the high-resolution laboratory absorption spectroscopy on low-J transitions in A 2Π(0,0,0)-X 2ς+(0,0,0) band of buffer-gas-cooled CaOH. In total, 40 transitions out of the low-J states were assigned, including 27 transitions that have not been reported in previous literature. The determined rotational constants for both ground and excited states are in excellent agreement with previous literature, and the measurement uncertainty for the absolute transition frequencies was improved by more than a factor of 3. This will aid future interstellar, circumstellar, and atmospheric identifications of CaOH. The buffer-gas-cooling method employed here is a particularly powerful method to probe low-J transitions and is easily applicable to other astrophysical molecules.
UR - http://www.scopus.com/inward/record.url?scp=85137776829&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/ac87fb
DO - 10.3847/1538-4357/ac87fb
M3 - 学術論文
AN - SCOPUS:85137776829
SN - 0004-637X
VL - 936
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 97
ER -