tipa -- 2/9/2017

A dearth of short-period massive binaries in the young massive star forming region M17: Evidence for a large orbital separation at birth?

• H. Sana, M. Ramirez-Tannus, A. de Koter, L. Kaper, F. Tramper, A. Bik

The ultracompact nature of the black hole candidate X-ray binary 47 Tuc X9

• Arash Bahramian, Craig O. Heinke, Vlad Tudor, James C.A. Miller-Jones, Slavko Bogdanov, Thomas J. Maccarone, Christian Knigge, Gregory R. Sivakoff, Laura Chomiuk, Jay Strader, Javier A. Garcia, Timothy Kallman

Magnetic Origin of Black Hole Winds Across the Mass Scale

• Keigo Fukumura, Demosthenes Kazanas, Chris Shrader, Ehud Behar, Francesco Tombesi, Ioannis Contopoulos

The Fan Region at 1.5 GHz. I: Polarized synchrotron emission extending beyond the Perseus Arm

• A. S. Hill, T. L. Landecker, E. Carretti, K. Douglas, X. H. Sun, B. M. Gaensler, S. A. Mao, N. M. McClure-Griffiths, W. Reich, M. Wolleben, J. M. Dickey, A. D. Gray, M. Haverkorn, J. P. Leahy, D. H. F. M. Schnitzeler

Possible pair-instability supernovae at solar metallicity from magnetic stellar progenitors

• Cyril Georgy, Georges Meynet, Sylvia Ekström, Gregg A. Wade, Véronique Petit, Zsolt Keszthelyi, Raphael Hirschi

Spectral energy distribution and radio halo of NGC253 at low radio frequencies

• A.D. Kapinska, L. Staveley-Smith, R. Crocker, G.R. Meurer, S. Bhandari, N. Hurley-Walker, A.R. Offringa, D.J. Hanish, N. Seymour, R.D. Ekers, M.E. Bell, J.R. Callingham, K.S. Dwarakanath, B.-Q. For, B. M. Gaensler, P.J. Hancock, L. Hindson, M. Johnston-Hollitt, E. Lenc, B. McKinley, J. Morgan, P. Procopio, R.B. Wayth, C. Wu, Q. Zheng, N. Barry, A.P. Beardsley, J.D. Bowman, F. Briggs, P. Carroll, J.S. Dillon, A. Ewall-Wice, L. Feng, L.J. Greenhill, B.J. Hazelton, J.N. Hewitt, D.J. Jacobs, H.-S. Kim, P. Kittiwisit, J. Line, A. Loeb, D.A. Mitchell, M.F. Morales, A.R. Neben, S. Paul, B. Pindor, J.C. Pober, J. Riding, S.K. Sethi, N. Udaya Shankar, R. Subrahmanyan, I.S. Sullivan, M. Tegmark, N. Thyagarajan, S.J. Tingay, C.M. Trott, R.L. Webster, S.B. Wyithe