Zobrazeno 1 - 10
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pro vyhledávání: '"Noel, D"'
Autor:
Richardson, Noel D., Schaefer, Gail H., Eldridge, Jan J., Spejcher, Rebecca, Holdsworth, Amanda, Lau, Ryan M., Monnier, John D., Moffat, Anthony F. J., Weigelt, Gerd, Williams, Peredur M., Kraus, Stefan, Bouquin, Jean-Baptiste Le, Anugu, Narsireddy, Chhabra, Sorabh, Codron, Isabelle, Ennis, Jacob, Gardner, Tyler, Gutierrez, Mayra, Ibrahim, Noura, Labdon, Aaron, Lanthermann, Cyprien, Setterholm, Benjamin R.
Classical Wolf-Rayet stars are the descendants of massive OB stars that have lost their hydrogen envelopes and are burning helium in their cores prior to exploding as type Ib/c supernovae. The mechanisms for losing their hydrogen envelopes are either
Externí odkaz:
http://arxiv.org/abs/2410.09259
Autor:
Richardson, Noel D., Daly, Andrea R., Williams, Peredur M., Hill, Grant M., Shenavrin, Victor I., Endo, Izumi, Chené, André-Nicolas, Karnath, Nicole, Lau, Ryan M., Moffat, Anthony F. J., Weigelt, Gerd
Several long-period binaries with a carbon-rich Wolf-Rayet star and an O star produce dust in their wind collisions. In eccentric binaries, this is seen most strongly near periastron passage. The exact conditions leading to dust creation require orbi
Externí odkaz:
http://arxiv.org/abs/2405.10454
Autor:
Gull, Theodore R., Hartman, Henrik, Corcoran, Michael F., Damineli, Augusto, Madura, Thomas, Moffat, Anthony F. J., Richardson, Noel D., Weigelt, Gerd
Eta Carinae underwent the Great Eruption in the 1840s and a Lesser Eruption in the 1890s. Its apparent spectrum, modified by intervening ejecta, the Homunculus and Little Homunculus, continues to evolve but contains information pertaining to events i
Externí odkaz:
http://arxiv.org/abs/2403.13954
Autor:
Damineli, Augusto, Richardson, Noel D., Navarete, Felipe, Gull, Theodore. R., Fernández-Lajús, Eduardo, Moffat, Anthony F. J., Hillier, Desmond J., Weigelt, Gerd, Corcoran, Michael F.
Changes in the flux and spectrum of Eta Carinae since 1900 have been attributed to the evolution of the central binary by some. Others suggest evolution in the occulting ejecta. The brightness jump in the 1940s, which coincided with the appearance of
Externí odkaz:
http://arxiv.org/abs/2312.17421
Autor:
Lau, Ryan M., Hankins, Matthew J., Sanchez-Bermudez, Joel, Thatte, Deepashri, Soulain, Anthony, Cooper, Rachel A., Sivaramakrishnan, Anand, Corcoran, Michael F., Greenbaum, Alexandra Z., Gull, Theodore R., Han, Yinuo, Jones, Olivia C., Madura, Thomas, Moffat, Anthony F. J., Morris, Mark R., Onaka, Takashi, Russell, Christopher M. P., Richardson, Noel D., Smith, Nathan, Tuthill, Peter, Volk, Kevin, Weigelt, Gerd, Williams, Peredur M.
We present infrared aperture masking interferometry (AMI) observations of newly formed dust from the colliding winds of the massive binary system Wolf-Rayet (WR) 137 with JWST using the Near Infrared Imager and Slitless Spectrograph (NIRISS). NIRISS
Externí odkaz:
http://arxiv.org/abs/2311.15948
Autor:
Pavao, Clarissa M., Richardson, Noel D., Labadie-Bartz, Jonathan, Pablo, Herbert, Chené, André-Nicolas
Be X-ray binaries (Be XRBs) are high-mass X-ray binaries, with a neutron star or black hole orbiting and accreting material from a non-supergiant B-star that is rotating at a near critical rate. These objects are prime targets to understand past bina
Externí odkaz:
http://arxiv.org/abs/2311.00293
Autor:
Barclay, Krister DG., Rosu, Sophie, Richardson, Noel D., Chené, André-Nicolas, St-Louis, Nicole, Ignace, Richard, Moffat, Anthony F. J.
The bright WN4 star EZ CMa exhibits a 3.77 day periodicity in photometry, spectroscopy, and polarimetry but the variations in the measurements are not strictly phase-locked, exhibiting changes in reference times, amplitudes, and the shape of the vari
Externí odkaz:
http://arxiv.org/abs/2310.15986
Autor:
Peatt, Megan J., Richardson, Noel D., Williams, Peredur M., Karnath, Nicole, Shenavrin, Victor I., Lau, Ryan M., Moffat, Anthony F. J., Weigelt, Gerd
WR 137 (HD 192641) is a binary system consisting of a carbon-rich Wolf-Rayet star and an Oe companion star in a 13-year orbit. Near periastron, the winds of the two stars collide and form carbonaceous dust. We obtained three mid-infrared grism spectr
Externí odkaz:
http://arxiv.org/abs/2308.11798
Autor:
Gull, Theodore R., Hartman, Henrik, Teodoro, Mairan, Hillier, D. John, Corcoran, Michael F., Damineli, Augusto, Hamaguchi, Kenji, Madura, Thomas, Moffat, Anthony F. J., Morris, Patrick, Richardson, Noel D., Stevens, Ian R., Weigelt, Gerd
Previous STIS long-slit observations of Eta Carinae identified numerous absorption features in both the stellar spectrum, and in the adjacent nebular spectra, along our line-of-sight. The absorption features became temporarily stronger when the ioniz
Externí odkaz:
http://arxiv.org/abs/2305.13216