Artículo
Supan, L.; Castelletti, G.; Supanitsky, A.D.; Burton, M.G.; Wong, G.F.; Braiding, C. "Natal molecular cloud of SNR Kes 41. Complete characterisation" (2018) Astronomy and Astrophysics. 619
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Abstract:
Using high-resolution data of the 12CO and 13CO (J = 1-0) line emission from the Mopra Southern Galactic Plane CO Survey in conjunction with neutral hydrogen observations from the Southern Galactic Plane Survey (SGPS) and mid-infrared Spitzer data, we have explored the large-scale environment of the supernova remnant Kes 41. On the basis of these data, we identified for the first time the parent cloud of Kes 41 in its whole extension and surveyed the HII regions, masers, and the population of massive young stellar objects in the cloud. The whole unveiled giant cloud, located at the kinematic distance of 12.0 ± 3.6 kpc, whose average total mass and size are ~10-30 × 105 M and ∼ 26′, also shines in γ-rays, as revealed by the Large Area Telescope on board the Fermi satellite. We determined a high average proton density ∼500-1000 cm-3 in the large molecular complex, of which protons from the neutral atomic and ionised gases comprise only ∼15%. © 2018 ESO.
Registro:
| Documento: | Artículo |
| Título: | Natal molecular cloud of SNR Kes 41. Complete characterisation |
| Autor: | Supan, L.; Castelletti, G.; Supanitsky, A.D.; Burton, M.G.; Wong, G.F.; Braiding, C. |
| Filiación: | CONICET, Universidad de Buenos Aires, Instituto de Astronomiá y Física Del Espacio, Buenos Aires, Argentina Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Buenos Aires, Argentina School of Physics, University of New South Wales, Sydney, NSW 2052, Australia Armagh Observatory and Planetarium, College Hill, Armagh, BT619DG, United Kingdom School of Computing Enginnering and Mathematics, Western Sydney University, Locked Bay 1797, Penrith, NSW 2751, Australia |
| Palabras clave: | Gamma rays: ISM; ISM: Individual objects: Kes 41; ISM: Supernova remnants; Gamma rays; Population statistics; Supernovae; Surveys; Galactic plane surveys; Gamma rays: isms; High resolution data; ISM: individual objects; ISM: supernova remnants; Large area telescopes; Molecular complexes; Young stellar objects; Density of gases |
| Año: | 2018 |
| Volumen: | 619 |
| DOI: | http://dx.doi.org/10.1051/0004-6361/201833183 |
| Título revista: | Astronomy and Astrophysics |
| Título revista abreviado: | Astron. Astrophys. |
| ISSN: | 00046361 |
| CODEN: | AAEJA |
| Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v619_n_p_Supan |
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Citas:
---------- APA ----------
Supan, L., Castelletti, G., Supanitsky, A.D., Burton, M.G., Wong, G.F. & Braiding, C. (2018) . Natal molecular cloud of SNR Kes 41. Complete characterisation. Astronomy and Astrophysics, 619.http://dx.doi.org/10.1051/0004-6361/201833183
---------- CHICAGO ----------
Supan, L., Castelletti, G., Supanitsky, A.D., Burton, M.G., Wong, G.F., Braiding, C. "Natal molecular cloud of SNR Kes 41. Complete characterisation" . Astronomy and Astrophysics 619 (2018).http://dx.doi.org/10.1051/0004-6361/201833183
---------- MLA ----------
Supan, L., Castelletti, G., Supanitsky, A.D., Burton, M.G., Wong, G.F., Braiding, C. "Natal molecular cloud of SNR Kes 41. Complete characterisation" . Astronomy and Astrophysics, vol. 619, 2018.http://dx.doi.org/10.1051/0004-6361/201833183
---------- VANCOUVER ----------
Supan, L., Castelletti, G., Supanitsky, A.D., Burton, M.G., Wong, G.F., Braiding, C. Natal molecular cloud of SNR Kes 41. Complete characterisation. Astron. Astrophys. 2018;619.http://dx.doi.org/10.1051/0004-6361/201833183
