Time-dependent visibility modelling of a relativistic jet in the X-ray binary MAXI J1803-298

Autor: C M Wood, J C A Miller-Jones, A Bahramian, S J Tingay, T D Russell, A J Tetarenko, D Altamirano, T Belloni, F Carotenuto, C Ceccobello, S Corbel, M Espinasse, R P Fender, E Körding, S Migliari, D M Russell, C L Sarazin, G R Sivakoff, R Soria, V Tudose

Publikováno v: Monthly Notices of the Royal Astronomical Society, 522, 70-89
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2023, 522 (1), pp.70-89. ⟨10.1093/mnras/stad939⟩
Monthly Notices of the Royal Astronomical Society, 522, 1, pp. 70-89

Tracking the motions of transient jets launched by low-mass X-ray binaries (LMXBs) is critical for determining the moment of jet ejection, and identifying any corresponding signatures in the accretion flow. However, these jets are often highly variab

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d7094d50330baa915fe5014b88e25c69
http://arxiv.org/abs/2303.15648

Linking the dust and chemical evolution: Taurus and Perseus -- New collisional rates for HCN, HNC, and their C, N, and H isotopologues

Autor: D. Navarro-Almaida, C. T. Bop, F. Lique, G. Esplugues, M. Rodríguez-Baras, C. Kramer, C. E. Romero, A. Fuente, P. Caselli, P. Rivière-Marichalar, J. M. Kirk, A. Chacón-Tanarro, E. Roueff, T. Mroczkowski, T. Bhandarkar, M. Devlin, S. Dicker, I. Lowe, B. Mason, C. L. Sarazin, J. Sievers

HCN, HNC, and their isotopologues are ubiquitous molecules that can serve as chemical thermometers and evolutionary tracers to characterize star-forming regions. Despite their importance in carrying information that is vital to studies of the chemist

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a9367746d5f77fde82676eee0fad543c

The Effect of SNR Structure on Non-equilibrium X-ray Spectra

Autor: A. J. S. Hamilton, C. L. Sarazin

Publikováno v: Symposium - International Astronomical Union. 101:113-118

A technique is presented for characterizing the ionization structure and consequent thermal x-ray emission of a SNR when non-equilibrium ionization effects are important. The technique allows different theoretical SNR models to be compared and contra

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::6258fbe2ae5451ea0f979f62f47104fb
https://doi.org/10.1017/s007418090003374x

Radio recombination lines from quasars. I - Level populations of hydrogenic ions in a strong, nonthermal radiation field

Autor: R. L. Brown, C. L. Sarazin, E. J. Wadiak

Publikováno v: The Astrophysical Journal Supplement Series. 53:351

On donne une vaste serie de modeles pour un domaine de valeurs de l'intensite et de l'indice spectral radio et de la temperature electronique et de la densite du gaz ionise. On considere l'effet des coupures a basse frequence dans le spectre de la ra

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::5009b0cc92ba86dc1bbb2476a06425b4
https://doi.org/10.1086/190894

The effect of multiple grain components on infrared radiation transfer and the 10 micron silicate feature

Autor: C. L. Sarazin

Publikováno v: The Astrophysical Journal. 220:165

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::98c5bb7e0e53024e79ea26739fc9f711
https://doi.org/10.1086/155892