Magnetic Stars, 2011, pp. ... It follows, in particular, from Fig. 1a, where points show the central intensity of line in 2008 ­ 2009, and asterisks -- the ELODIE Archive (EA) spectra in 2002 ­ 2003 smoothed to the resolution of the MSS. ... Figure 2a demonstrates the distribution of temperature in the atmosphere in the phase = 0.07 and Fig. 2b -- in the phase = 0.53 of the rotation period, obtained from the hydrogen line profiles in 2008 ­ 2009. ...

PSR: J1842-0359 B1839-04 Scode: 100 RAB: 18:39:48.10000 +/- 00:00:00.09997 DECB: -04:02:58.0000 +/- 00:00:02.9908 RAJ: 18:42:26.49144 +/- 00:00:00.09997 DECJ: -03:59:59.1614 +/- 00:00:02.9908 l,b: 28.347 0.174 P: 1.839944207000000054 +/- 0.000000000200000000 Pdot: 5.100000E-16 +/- 1.000000E-17 Pepoch: 47000. DM: 196.0000 +/- 12.0000 w50: 262.00 ms 142.40 mP s400: 18.70 s1400: 8.50 RM: 326.00 +/- 9.00 log tau_s: -1.70 d,z: 4.15 0.01 aa model d: 4.15 (model 1) L: 2.51 age: 7.76 Edot: 30.51 B: 11.99