机译:DO光谱致密气体级分轨道分子云表面密度吗?
Department of Astronomy The Ohio State University 4055 McPherson Laboratory 140 West 18th Avenue Columbus OH 43210 USA;
Department of Astronomy The Ohio State University 4055 McPherson Laboratory 140 West 18th Avenue Columbus OH 43210 USA;
AIfA Universit?t Bonn Auf dem Hügel 71 D-53121 Bonn Germany;
AIM CEA CNRS Université Paris-Saclay Université Paris Diderot Sorbonne Paris Cité F-91191 Gif-sur-Yvette France;
Harvard-Smithsonian Center for Astrophysics 60 Garden Street Cambridge MA 02138 USA;
CNRS IRAP 9 av. du Colonel Roche BP 44346 F-31028 Toulouse cedex 4 France;
Institut de Radioastronomie Millimètrique (IRAM) 300 Rue de la Piscine F-38406 Saint Martin d'Hères France;
Max Planck Institute für Astronomie K?nigstuhl 17 D-69117 Heidelberg Germany;
Department of Astronomy The Ohio State University 4055 McPherson Laboratory 140 West 18th Avenue Columbus OH 43210 USA;
Observatorio Astronómico Nacional (IGN) C/Alfonso XII 3 E-28014 Madrid Spain;
Department of Astronomy The Ohio State University 4055 McPherson Laboratory 140 West 18th Avenue Columbus OH 43210 USA;
Department of Astronomy University of Maryland College Park MD 20742-2421 USA;
Astronomisches Rechen-Institut Zentrum für Astronomie der Universit?t Heidelberg M?nchhofstra?e 12-14 D-69120 Heidelberg Germany;
Max Planck Institute für Astronomie K?nigstuhl 17 D-69117 Heidelberg Germany;
Institute für theoretische Astrophysik Zentrum für Astronomie der Universit?t Heidelberg Albert-Ueberle Str. 2 D-69120 Heidelberg Germany;
National Radio Astronomy Observatory 520 Edgemont Road Charlottesville VA 22903-2475 USA;
Astronomisches Rechen-Institut Zentrum für Astronomie der Universit?t Heidelberg M?nchhofstra?e 12-14 D-69120 Heidelberg Germany;
Research School of Astronomy &
Astrophysics Australian National University Canberra ACT 2611 Australia;
Max Planck Institute für Astronomie K?nigstuhl 17 D-69117 Heidelberg Germany;
Department of Physics New Mexico Institute of Mining and Technology 801 Leroy Place Soccoro NM 87801 USA;
National Radio Astronomy Observatory 520 Edgemont Road Charlottesville VA 22903-2475 USA;
Observatorio Astronómico Nacional (IGN) C/Alfonso XII 3 E-28014 Madrid Spain;
Department of Physics University of Alberta Edmonton AB T6G 2E1 Canada;
Max Planck Institute für Astronomie K?nigstuhl 17 D-69117 Heidelberg Germany;
Max-Planck-Institut für extraterrestrische Physik Giessenbachstra?e 1 D-85748 Garching Germany;
galaxies; ISM - galaxies; star formation - ISM; clouds - ISM; molecules - ISM; structure;
机译:DO光谱致密气体级分轨道分子云表面密度吗?
机译:大型麦哲伦云中巨大分子云的密集簇:从13CO(J = 3-2)观察得出的密度和温度
机译:大型麦哲伦云中巨大分子云的密集簇:从13CO(J = 3-2)观察得出的密度和温度
机译:帕金森药物2-(3,4-二羟基苯基)乙胺密度函数理论的分子对接和光谱研究辅助
机译:使用重气萃取按分子量分馏碳质沥青
机译:致密分子云中的氧分馏
机译:致密分子云中碳分馏的气体晶粒模型
机译:三氟氯乙烯聚合物的物理性质与分子量的关系。 2.三氟氯乙烯聚合物的分子分馏,密度,粘度,分子量和这些性质的相关性