METHANIMINE IN COOL COSMIC OBJECTS USING ACCURATE COLLISIONAL RATE COEFFICIENTS

被引:0
作者
Chandra, S. [1 ]
Sharma, M. K. [2 ]
机构
[1] Amity Univ Uttar Pradesh, Amity Inst Appl Sci, Amity Ctr Astron & Astrophys, Sect 125, Noida 201313, India
[2] Sunder Deep Grp Inst, Dept Phys, NH-24,Delhi Hapur Rd, Dasna 201001, India
关键词
ISM; molecules; methanimine; MASER action and radiative transfer; INTERSTELLAR METHANIMINE; MICROWAVE DETECTION; SAGITTARIUS B2; LINE SURVEY; CH2NH; HYDROGENATION; METHYLENEIMINE; MOLECULES; DISCOVERY; GLYCINE;
D O I
10.1007/s10511-024-09838-x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Accurate collisional rate coefficients for collisional transitions between 15 rotational levels of methanimine, colliding with p-H-2 molecule, are available. Methanimine is a planar, asymmetric top molecule having electric dipole moment with components mu(a) = 1.3396 Debye and mu(b) = 1.4461 Debye, and thus, producing both the a and b type spectral lines of nearly equal intensities. Therefore, all the rotational levels need to be considered together. Between 15 rotational levels, 105 collisional transitions are considered in an investigation by others. We have discussed that each level is not connected with all others through the collisions, and therefore, there should be 77 instead of 105 collisional transitions between 15 levels of methanimine. With availability of accurate collisional rate coefficients, it is worth to perform the Sobolev analysis of methanimine. We have found six weak MASER transitions, 1(10)-1(11), 2(11)-2(12), 3(12)-3(13), 4(1.3)-4(1.4), 3(03)-2(12) and 4(0.4)-3(1.3), and one transition 1(11)-2(02), showing anomalous absorption. These seven lines may play important role for the methanimine.
引用
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页码:364 / 374
页数:11
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