Works matching AU Esimbek, J.

Results: 11

DETERMINATION OF PHYSICAL PARAMETERS OF THE W40 HII REGION USING OBSERVATIONS OF Н110𝛼 RADIO RECOMBINATION LINE.

Published in:

Recent Contributions to Physics, 2023, v. 86, n. 3, p. 4, doi. 10.26577/RCPh.2023.v86.i3.01

By:

Manapbayeva, A. B.;
Omar, A. Zh.;
Alimgazinova, N. Sh.;
Komesh, T.;
Kyzgarina, M. T.;
Esimbek, J.;
Assembay, Zh.

Publication type:

Article

ALMA observations of the environments of G301.1364-00.2249A.

Published in:

Proceedings of the International Astronomical Union, 2022, v. 18, n. S380, p. 204, doi. 10.1017/S1743921323002624

By:

Assembay, Zh.;
Komesh, T.;
Garay, G.;
Omar, A.;
Esimbek, J.;
Alimgazinova, N.;
Kyzgarina, M.;
Murat, Sh.

Publication type:

Article

ALMA view of the 12C/13C isotopic ratio in starburst galaxies.

Published in:

Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 629, p. 1, doi. 10.1051/0004-6361/201935603

By:

Tang, X. D.;
Henkel, C.;
Menten, K. M.;
Gong, Y.;
Martín, S.;
Mühle, S.;
Aalto, S.;
Muller, S.;
García-Burillo, S.;
Levshakov, S.;
Aladro, R.;
Spaans, M.;
Viti, S.;
Asiri, H. M.;
Ao, Y. P.;
Zhang, J. S.;
Zheng, X. W.;
Esimbek, J.;
Zhou, J. J.

Publication type:

Article

ATLASGAL-selected massive clumps in the inner Galaxy: VI. Kinetic temperature and spatial density measured with formaldehyde.

Published in:

Astronomy & Astrophysics / Astronomie et Astrophysique, 2018, v. 611, p. 1, doi. 10.1051/0004-6361/201732168

By:

Tang, X. D.;
Henkel, C.;
Wyrowski, F.;
Giannetti, A.;
Menten, K. M.;
Csengeri, T.;
Leurini, S.;
Urquhart, J. S.;
König, C.;
Güsten, R.;
Lin, Y. X.;
Zheng, X. W.;
Esimbek, J.;
Zhou, J. J.

Publication type:

Article

Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde III. The Orion molecular cloud 1.

Published in:

Astronomy & Astrophysics / Astronomie et Astrophysique, 2018, v. 609, p. 1, doi. 10.1051/0004-6361/201731849

By:

Tang, X. D.;
Henkel, C.;
Menten, K. M.;
Wyrowski, F.;
Brinkmann, N.;
Zheng, X. W.;
Gong, Y.;
Lin, Y. X.;
Esimbek, J.;
Zhou, J. J.;
Yuan, Y.;
Li, D. L.;
He, Y. X.

Publication type:

Article

Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde: II. The Large Magellanic Cloud.

Published in:

Astronomy & Astrophysics / Astronomie et Astrophysique, 2017, v. 600, p. 1, doi. 10.1051/0004-6361/201630183

By:

Tang, X. D.;
Henkel, C.;
Chen, C.-H. R.;
Menten, K. M.;
Indebetouw, R.;
Zheng, X. W.;
Esimbek, J.;
Zhou, J. J.;
Yuan, Y.;
Li, D. L.;
He, Y. X.

Publication type:

Article

Filament L1482 in the California molecular cloud.

Published in:

Astronomy & Astrophysics / Astronomie et Astrophysique, 2014, v. 567, p. 1, doi. 10.1051/0004-6361/201323122

By:

Li, D. L.;
Esimbek, J.;
Zhou, J. J.;
Lou, Y.-Q.;
Wu, G.;
Tang, X. D.;
He, Y. X.

Publication type:

Article

The relation of H2CO, 12CO, and 13CO in molecular clouds.

Published in:

Astronomy & Astrophysics / Astronomie et Astrophysique, 2013, v. 551, p. 1, doi. 10.1051/0004-6361/201219809

By:

X. D. Tang;
J. Esimbek;
J. J. Zhou;
G.Wu;
W. G. Ji;
Okoh, D.

Publication type:

Article

The infrared dust bubble N22: an expanding H II region and the star formation around it.

Published in:

Astronomy & Astrophysics / Astronomie et Astrophysique, 2012, v. 544, n. 1, p. 1, doi. 10.1051/0004-6361/201218861

By:

W.-G. Ji;
J.-J. Zhou;
Esimbek, J.;
Y.-F. Wu;
G. Wu;
X.-D. Tang

Publication type:

Article

Molecular clouds at the edge of the Galaxy: I. Variation in the CO J = 2–1/1–0 line ratio.

Published in:

Astronomy & Astrophysics / Astronomie et Astrophysique, 2025, v. 698, p. 1, doi. 10.1051/0004-6361/202453007

By:

Luo, C. S.;
Tang, X. D.;
Henkel, C.;
Menten, K. M.;
Sun, Y.;
Gong, Y.;
Zheng, X. W.;
Li, D. L.;
He, Y. X.;
Lu, X.;
Ao, Y. P.;
Chen, X. P.;
Liu, T.;
Wang, K.;
Wu, J. W.;
Esimbek, J.;
Zhou, J. J.;
Qiu, J. J.;
Zhao, X.;
Li, J. S.

Publication type:

Article

Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde: V. The massive filament DR21.

Published in:

Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202449352

By:

Zhao, X.;
Tang, X. D.;
Henkel, C.;
Gong, Y.;
Lin, Y.;
Li, D. L.;
He, Y. X.;
Ao, Y. P.;
Lu, X.;
Liu, T.;
Sun, Y.;
Wang, K.;
Chen, X. P.;
Esimbek, J.;
Zhou, J. J.;
Wu, J. W.;
Qiu, J. J.;
Zheng, X. W.;
Li, J. S.;
Luo, C. S.

Publication type:

Article

Works matching AU Esimbek, J.

DETERMINATION OF PHYSICAL PARAMETERS OF THE W40 HII REGION USING OBSERVATIONS OF Н110𝛼 RADIO RECOMBINATION LINE.

ALMA observations of the environments of G301.1364-00.2249A.

ALMA view of the <sup>12</sup>C/<sup>13</sup>C isotopic ratio in starburst galaxies.

ATLASGAL-selected massive clumps in the inner Galaxy: VI. Kinetic temperature and spatial density measured with formaldehyde.

Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde III. The Orion molecular cloud 1.

Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde: II. The Large Magellanic Cloud.

Filament L1482 in the California molecular cloud.

The relation of H<sub>2</sub>CO, <sup>12</sup>CO, and <sup>13</sup>CO in molecular clouds.

The infrared dust bubble N22: an expanding H II region and the star formation around it.

Molecular clouds at the edge of the Galaxy: I. Variation in the CO J = 2–1/1–0 line ratio.

Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde: V. The massive filament DR21.