Zobrazeno 1 - 10
of 41
pro vyhledávání: '"Carter, Bradley D."'
Autor:
Evensberget, Dag, Marsden, Stephen C., Carter, Bradley D., Salmeron, Raquel, Vidotto, Aline A., Folsom, Colin P., Kavanagh, Robert D., Driessen, Florian A., Strickert, K. Markus
Solar-type stars, which shed angular momentum via magnetised stellar winds, enter the main sequence with a wide range of rotational periods $P_\text{rot}$. This initially wide range of rotational periods contracts and has mostly vanished by a stellar
Externí odkaz:
http://arxiv.org/abs/2305.17427
Autor:
Zeng, Yunlin, Brandt, Timothy D., Li, Gongjie, Dupuy, Trent J., Li, Yiting, Brandt, G. Mirek, Farihi, Jay, Horner, Jonathan, Wittenmyer, Robert A., Butler, R. Paul., Tinney, Christopher G., Carter, Bradley D., Wright, Duncan J., Jones, Hugh R. A., O'Toole, Simon J.
Gliese 86 is a nearby K dwarf hosting a giant planet on a $\approx$16-day orbit and an outer white dwarf companion on a $\approx$century-long orbit. In this study we combine radial velocity data (including new measurements spanning more than a decade
Externí odkaz:
http://arxiv.org/abs/2112.06394
Autor:
Evensberget, Dag, Carter, Bradley D., Marsden, Stephen C., Brookshaw, Leigh, Folsom, Colin P., Salmeron, Raquel
We present wind models of ten young Solar-type stars in the Hercules-Lyra association and the Coma Berenices cluster aged around 0.26 Gyr and 0.58 Gyr respectively. Combined with five previously modelled stars in the Hyades cluster, aged 0.63 Gyr, we
Externí odkaz:
http://arxiv.org/abs/2112.01445
Autor:
Evensberget, Dag, Carter, Bradley D., Marsden, Stephen C., Brookshaw, Leigh, Folsom, Colin P.
Stellar winds govern the spin-down of Solar-type stars as they age, and play an important role in determining planetary habitability, as powerful winds can lead to atmospheric erosion. We calculate three-dimensional stellar wind models for five young
Externí odkaz:
http://arxiv.org/abs/2106.04937
Autor:
Addison, Brett C., Wright, Duncan J., Nicholson, Belinda A., Cale, Bryson, Mocnik, Teo, Huber, Daniel, Plavchan, Peter, Wittenmyer, Robert A., Vanderburg, Andrew, Chaplin, William J., Chontos, Ashley, Clark, Jake T., Eastman, Jason D., Ziegler, Carl, Brahm, Rafael, Carter, Bradley D., Clerte, Mathieu, Espinoza, Néstor, Horner, Jonathan, Bentley, John, Jordán, Andrés, Kane, Stephen R., Kielkopf, John F., Laychock, Emilie, Mengel, Matthew W., Okumura, Jack, Stassun, Keivan G., Bedding, Timothy R., Bowler, Brendan P., Burnelis, Andrius, Blanco-Cuaresma, Sergi, Collins, Michaela, Crossfield, Ian, Davis, Allen B., Evensberget, Dag, Heitzmann, Alexis, Howell, Steve B., Law, Nicholas, Mann, Andrew W., Marsden, Stephen C., Matson, Rachel A., O'Connor, James, Shporer, Avi, Stevens, Catherine, Tinney, C. G., Tylor, Christopher, Wang, Songhu, Zhang, Hui, Henning, Thomas, Kossakowski, Diana, Ricker, George, Sarkis, Paula, Schlecker, Martin, Torres, Pascal, Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Mireles, Ismael, Rowden, Pam, Pepper, Joshua, Daylan, Tansu, Schlieder, Joshua E., Collins, Karen A., Collins, Kevin I., Tan, Thiam-Guan, Ball, Warrick H., Basu, Sarbani, Buzasi, Derek L., Campante, Tiago L., Corsaro, Enrico, González-Cuesta, Lucía, Davies, Guy R., de Almeida, Leandro, Nascimento, Jr., Jose-Dias do, a, Rafael A. Garcí, Guo, Zhao, Handberg, Rasmus, Hekker, Saskia, Hey, Daniel R., Kallinger, Thomas, Kawaler, Steven D., Kayhan, Cenk, Kuszlewicz, James S., Lund, Mikkel N., Lyttle, Alexander, Mathur, Savita, Miglio, Andrea, Mosser, Benoit, Nielsen, Martin B., Serenelli, Aldo M., Aguirre, Victor Silva, Themeßl, Nathalie
We report the discovery of a warm sub-Saturn, TOI-257b (HD 19916b), based on data from NASA's Transiting Exoplanet Survey Satellite (TESS). The transit signal was detected by TESS and confirmed to be of planetary origin based on radial velocity obser
Externí odkaz:
http://arxiv.org/abs/2001.07345
We report the observation on UT 2017.07.01 of an unusually powerful flare detected in near-infrared continuum photometry of Proxima Centauri. During a campaign monitoring the star for possible exoplanet transits, we identified an increase in Sloan i'
Externí odkaz:
http://arxiv.org/abs/1904.06875
Autor:
Addison, Brett, Wright, Duncan J., Wittenmyer, Robert A., Horner, Jonathan, Mengel, Matthew W., Johns, Daniel, Marti, Connor, Nicholson, Belinda, Okumura, Jack, Bowler, Brendan, Crossfield, Ian, Kane, Stephen R., Kielkopf, John, Plavchan, Peter, Tinney, C. G., Zhang, Hui, Clark, Jake T., Clerte, Mathieu, Eastman, Jason D., Swift, Jon, Bottom, Michael, Muirhead, Philip, McCrady, Nate, Herzig, Erich, Hogstrom, Kristina, Wilson, Maurice, Sliski, David, Johnson, Samson A., Wright, Jason T., Blake, Cullen, Riddle, Reed, Lin, Brian, Cornachione, Matthew, Bedding, Timothy R., Stello, Dennis, Huber, Daniel, Marsden, Stephen, Carter, Bradley D.
Publikováno v:
Publications of the Astronomical Society of the Pacific, Volume 131, Issue 1005, pp. 115003 (2019)
The Minerva-Australis telescope array is a facility dedicated to the follow-up, confirmation, characterisation, and mass measurement of bright transiting planets discovered by the Transiting Exoplanet Survey Satellite (TESS) -- a category in which it
Externí odkaz:
http://arxiv.org/abs/1901.11231
Autor:
Cotton, Daniel V., Evensberget, Dag, Marsden, Stephen C., Bailey, Jeremy, Zhao, Jinglin, Kedziora-Chudczer, Lucyna, Carter, Bradley D., Bott, Kimberly, Vidotto, Aline A., Petit, Pascal, Morin, Julien, Jeffers, Sandra V.
We have observed the active star $\xi$ Boo A (HD 131156A) with high precision broadband linear polarimetry contemporaneously with circular spectropolarimetry. We find both signals are modulated by the 6.43 day rotation period of $\xi$ Boo A. The sign
Externí odkaz:
http://arxiv.org/abs/1811.08534
Autor:
Cotton, Daniel V., Marshall, Jonathan P., Bailey, Jeremy, Kedziora-Chudczer, Lucyna, Bott, Kimberly, Marsden, Stephen C., Carter, Bradley D.
We present linear polarization measurements of nearby FGK dwarfs to parts-per-million (ppm) precision. Before making any allowance for interstellar polarization, we found that the active stars within the sample have a mean polarization of 28.5 +/- 2.
Externí odkaz:
http://arxiv.org/abs/1701.02890
Autor:
Addison, Brett, Wright, Duncan J., Wittenmyer, Robert A., Horner, Jonathan, Mengel, Matthew W., Johns, Daniel, Marti, Connor, Nicholson, Belinda, Soutter, Jack, Bowler, Brendan, Crossfield, Ian, Kane, Stephen R., Kielkopf, John, Plavchan, Peter, Tinney, C. G., Zhang, Hui, Clark, Jake T., Clerte, Mathieu, Eastman, Jason D., Swift, Jon, Bottom, Michael, Muirhead, Philip, McCrady, Nate, Herzig, Erich, Hogstrom, Kristina, Wilson, Maurice, Sliski, David, Johnson, Samson A., Wright, Jason T., Johnson, John Asher, Blake, Cullen, Riddle, Reed, Lin, Brian, Cornachione, Matthew, Bedding, Timothy R., Stello, Dennis, Huber, Daniel, Marsden, Stephen, Carter, Bradley D.
Publikováno v:
Publications of the Astronomical Society of the Pacific, 2019 Nov 01. 131(1005), 1-15.
Externí odkaz:
https://www.jstor.org/stable/26973205
