Organisation profile

Organisation profile

CAR carries out research on a broad range of key science questions in astronomy.

Our research programmes mainly feature observational astronomy, and span the electromagnetic spectrum from X-rays to radio wavelengths. We study many sizescales, ranging from the properties of dust grains, up through stars and exoplanets through to entire galaxies and clusters of galaxies inthe near- and high-redshift Universe. Survey astronomy is a particularstrength. Our computing facilities also permit extensive in-house computer modelling and simulation, and we have a trackrecord of instrument development for astronomical polarimetry.

Our research performed well in RAE 2008, with the majority of our researchers rated as world-leading or internationally excellent.

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Collaborations and top research areas from the last five years

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  • Are Odd Radio Circles phoenixes of powerful radio galaxies?

    Shabala, S., Yates-Jones, P., Jerrim, L., Turner, R., Krause, M., Norris, R., Koribalski, B., Filipovic, M., Rudnick, L., Power, C. & Crocker, R., 15 Feb 2024, (Accepted/In press) In: Publications of the Astronomical Society of Australia.

    Research output: Contribution to journalArticlepeer-review

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  • On the Evolutionary History of a Simulated Disk Galaxy as Seen by Phylogenetic Trees

    de Brito Silva, D., Jofré, P., Tissera, P. B., Yaxley, K. J., Jara, J. G., Eldridge, C. J. L., Sillero, E., Yates, R. M., Hua, X., Das, P., Aguilera-Gómez, C., Johnston, E. J., Rojas-Arriagada, A., Foley, R. & Gilmore, G., 15 Feb 2024, In: The Astrophysical Journal. 962, 2, p. 1-18 18 p., 154.

    Research output: Contribution to journalArticlepeer-review

    Open Access
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  • Filamentary Network and Magnetic Field Structures Revealed with BISTRO in the High-mass Star-forming Region NGC 2264: Global Properties and Local Magnetogravitational Configurations

    Wang, J-W., Koch, P. M., Clarke, S. D., Fuller, G., Peretto, N., Tang, Y-W., Yen, H-W., Lai, S-P., Ohashi, N., Arzoumanian, D., Johnstone, D., Furuya, R., Inutsuka, S., Lee, C. W., Ward-Thompson, D., Le Gouellec, V. J. M., Liu, H-L., Fanciullo, L., Hwang, J., Pattle, K., & 137 othersPoidevin, F., Tahani, M., Onaka, T., Rawlings, M. G., Chung, E. J., Liu, J., Lyo, A-R., Priestley, F., Hoang, T., Tamura, M., Berry, D., Bastien, P., Ching, T-C., Coudé, S., Kwon, W., Chen, M., Eswaraiah, C., Soam, A., Hasegawa, T., Qiu, K., Bourke, T. L., Byun, D-Y., Chen, Z., Chen, H-R. V., Chen, W. P., Cho, J., Choi, M., Choi, Y., Choi, Y., Chrysostomou, A., Dai, S., Di Francesco, J., Diep​, P. N., Doi, Y., Duan, Y., Duan, H-Y., Eden, D., Fiege, J., Fissel, L. M., Franzmann, E., Friberg, P., Friesen, R., Gledhill, T., Graves, S., Greaves, J., Griffin, M., Gu, Q., Han, I., Hayashi, S., Houde, M., Inoue, T., Iwasaki, K., Jeong, I-G., Könyves, V., Kang, J., Kang, M., Karoly, J., Kataoka, A., Kawabata, K., Khan, Z., Kim, M-R., Kim, K-T., Kim, K. H., Kim, S., Kim, J., Kim, H., Kim, G., Kirchschlager, F., Kirk, J., Kobayashi, M. I. N., Kusune, T., Kwon, J., Lacaille, K., Law, C-Y., Lee, S-S., Lee, H., Lee, J-E., Lee, C-F., Li, D., Li, H., Li, G., Li, D., Lin, S-J., Liu, T., Liu, S-Y., Lu, X., Mairs, S., Matsumura, M., Matthews, B., Moriarty-Schieven, G., Nagata, T., Nakamura, F., Nakanishi, H., Ngoc, NB., Park, G., Parsons, H., Pyo, T-S., Qian, L., Rao, R., Rawlings, J., Retter, B., Richer, J., Rigby, A., Sadavoy, S., Saito, H., Savini, G., Seta, M., Sharma, E., Shimajiri, Y., Shinnaga, H., Tang, X., Thuong, H. D., Tomisaka, K., Tram, L. N., Tsukamoto, Y., Viti, S., Wang, H., Whitworth, A., Wu, J., Xie, J., Yang, M-Z., Yoo, H., Yuan, J., Yun, H-S., Zenko, T., Zhang, C-P., Zhang, Y., Zhang, G., Zhou, J., Zhu, L., de Looze, I., André, P., Dowell, C. D., Eyres, S., Falle, S., Robitaille, J-F. & van Loo, S., 14 Feb 2024, In: The Astrophysical Journal. 962, 2, p. 1-34 34 p., 136.

    Research output: Contribution to journalArticlepeer-review

    Open Access
    File
    2 Downloads (Pure)