Zobrazeno 1 - 10
of 537
pro vyhledávání: '"Bowler M"'
Autor:
Bowler, M. G.
Publikováno v:
Galaxies 2021 9 46
Abstract The microquasar SS 433 exhibits in H alpha intermittent flares, Doppler shifted to both the red and the blue. The mean remembers the orbital phase of the compact object. I show that the flares are not intermittent sightings of an accretion d
Externí odkaz:
http://arxiv.org/abs/2103.15782
Autor:
Bowler, M. G.
The Galactic microquasar SS 433 is a member of a binary system but there is a lack of data on the orbital velocities of the components. The emission lines of the C II doublet at 7231 and 7236 Angstrom have been tracked nightly over two orbital cycles
Externí odkaz:
http://arxiv.org/abs/2009.00589
Autor:
Bowler, M. G.
Publikováno v:
Particles 2024 7 805
The jets of SS 433 have punched through the supernova remnant from the explosion forming the compact object. The precessing jets collimate before reaching beyond the shell, some 40 pc downstream, just the region of origin of TeV gamma radiation. Coll
Externí odkaz:
http://arxiv.org/abs/2008.10042
Autor:
Bowler, M G
Two recent and robust determinations of the mass ratio agree on a value 0.7
Comment: 6 pages, 2 figures
Comment: 6 pages, 2 figures
Externí odkaz:
http://arxiv.org/abs/1808.03502
Autor:
Bowler, M. G.
I discuss two points concerning recent Brackett series spectra of SS 433. The first is that outbursts to red and blue episodic in the Balmer series are now shown to be episodic in the far infrared Brackett series. The second point is that while in qu
Externí odkaz:
http://arxiv.org/abs/1708.02555
Autor:
Bowler, M G
Publikováno v:
Eur.J.Phys. 38 (2017) 055102
The proper application of the virial theorem to the origin of osmotic pressure provides a simple, vivid and complete explanation of the physical processes involved; osmosis is driven by differential solvent pressures. This simple and intuitive notion
Externí odkaz:
http://arxiv.org/abs/1608.00106
Autor:
Bowler, M G
Atomic oxygen emission at 8446 Angstroms traces the stable circumbinary disk undisturbed through an optical outburst and accompanying radio flare
Comment: The revised version of 2021 differs from the original in the addition of two figures and a
Comment: The revised version of 2021 differs from the original in the addition of two figures and a
Externí odkaz:
http://arxiv.org/abs/1512.06885
Autor:
Bowler, M. G.
Some stationary lines in the emission spectra of SS 433 are eclipsed, but most are not. Lines attributed to a circumbinary disk are not eclipsed, but double in relative intensity during primary eclipse. A C II doublet is eclipsed and Doppler shifts o
Externí odkaz:
http://arxiv.org/abs/1510.03667
Autor:
Recharte, M.1 (AUTHOR), Lee, P.1 (AUTHOR), Meza, D.2 (AUTHOR), Vick, S.‐J.1 (AUTHOR), Bowler, M.3 (AUTHOR) m.bowler@uos.ac.uk
Publikováno v:
Animal Conservation. Aug2024, Vol. 27 Issue 4, p566-579. 14p.
Autor:
Bowler, M G
Publikováno v:
A & A 556 A 149 (2013) July 2013
The H and He emission lines of the microquasar SS 433 contain features that look very like emission from a circumbinary ring. Phenomenological models have been successful but contain certain ad hoc features. In this note the lines are treated as reco
Externí odkaz:
http://arxiv.org/abs/1304.0354