*** News from VSNET *** The SU UMa-type dwarf nova 1RXP J113123+4322.5 is now in superoutburst, showing the period increase of superhumps. For more detail information about these objects, see below, "VSNET Weekly Campaign Summary" of the last week. --------------------------------------------------------------------------- VSNET (Variable Star Network) is an international variable star observing network, covering various areas of novae, supernovae, cataclysmic variables (CVs), X-ray transients, and other classical eruptive, pulsating, and eclipsing variables. VSNET is one of invited contributing organizations to the SkyPub AstroAlert system. The "News from VSNET", mainly focusing on recent remarkable activities of CVs and related systems, is issued on a weekly basis, except on occasions of extremely urgent or transient events. Please refer to the VSNET Home Page for more details of events and objects listed. VSNET Home Page: http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/ VSNET provides a number of mailing lists, on which various news and topics are discussed. Subscriptions to the VSNET mailing lists are free of charge; please refer to the instruction on the above page if a reader needs more information of the list structure. CCD observations of such targets are a relatively easy task for a 20-40cm telescope; simply take as many CCD frames (with exposure times 10-30 sec) as possible, spanning several hours per night. The only requirements are the weather and your patience! If you need more help on the observing technique, please feel free to ask on the vsnet-campaign list. We would sincerely appreciate volunteers who would join the VSNET Collaboration team to study the wonders of these exotic variable stars. To join the VSNET campaign collaborative list, send an e-mail to vsnet-adm@kusastro.kyoto-u.ac.jp (VSNET administrator) with a line "SUBSCRIBE vsnet-campaign." (VSNET campaign members are strongly recommended to subscribe to vsnet-alert at the same time). Regards, Taichi Kato On behalf of the VSNET administrator team ---------------------------------------------------------------------------- The following was issued on March 17, 2003, as VSNET campaign circulation 1376 [Note a large part of detailed information is posted to vsnet-campaign sub-lists]. VSNET Weekly Campaign Summary *** Last week news *** (new targets) 1RXP J113123+4322.5 (RA = 11h31m22s.426, Dec = +43d22'38".51) P. Schmeer reported an outburst (12.9mag) of this SU UMa-type dwarf nova on March 13 (vsnet-campaign-dn 3533, 3535, 3536). The Kyoto observation on March 13 revealed the presence of superhumps (amplitude 0.22 mag). The outburst was thus confirmed to be a genuine superoutburst. The object may have been on its final rising stage. The superhump period based on this single night observation is 0.0643(4) d, which may be slightly shorter than the one (0.06495 d) obtained in 2002 (vsnet-campaign-dn 3540). Combined with light curves on March 14, superhumps showed a slightly decrease of amplitude and a refined period of 0.06487(5) d (vsnet-campaign-dn 3541). T. Kato reported on March 17 that the superhump period increased to 0.06499(1) d (vsnet-campaign-dn 3545, 3546). The superoutburst continues (vsnet-campaign-dn 3543). SN 2003bt (RA = 10h55m22s.48, Dec = -07d39'12".3) SN 2003bt is hosted by MCG -01-28-006, a face-on barred-spiral galaxy. The new object is superimposed on the western arm. The expected maximum for typical SN Ia is consistent with the discovery magnitude (16.7mag)(vsnet-campaign-sn 578). The CfA team revealed that it was a type Ia SN about 2 weeks after maximum on Mar. 11.25 (vsnet-campaign-sn 580). BR Lup (RA = 15h35m51s.61, Dec = -40d34'25".4) R. Stubbings reported that BR Lup was in outburst (14.4mag) on March 10 (vsnet-campaign-dn 3528). V1333 Aql (RA = 19h11m16s.09, Dec = +00d35'06".0) S. A. Ilovaisky et al. reported that V1333 Aql = Aql X-1 was very bright at a maximum brightness V=16.2 on March 4-10. This is typical of the maximum levels reached during the large 1995 and 1998 outbursts (vsnet-campaign-xray 199). V568 Cyg (RA = 20h42m22s.3, Dec = +35d27'22") According to Y. Watanabe, the Be-star V568 Cyg is gradually brightening (vsnet-campaign-be 226). SN 2003bu (RA = 14h00m31s.45, Dec = -28d52'32".7) SN 2003bu is hosted by NGC 5393, a face-on barred spiral galaxy with ring structure. The SN is superimposed on the west end of the bar. The expected maximum for typical SN Ia is mag about 16.3 (vsnet-campaign-sn 581). 4U 1608-522 = QX Nor (RA = 16h12m42s.6, Dec = -52d25'21") According to ATEL #126 (Miller et al.), this X-ray transient (neutron star transient) is in outburst, based on RXTE/ASM observations (vsnet-campaign-xray 200). SN 2003bv (RA = 07h22m11s.92, Dec = +40d28'01".5) SN 2003bv is hosted by MCG +07-15-15, a barred-spiral galaxy with a ring structure. The expected maximum (derived from NED recession velocity) of typical SN Ia is well below (more than 1 mag) of the reported magnitude on Mar. 13.918 (16.8mag), so the timely follow-up observations (spectroscopy, photometry) are extremely encouraged (vsnet-campaign-sn 582). SN 2003bw (RA = 14h57m22s.44, Dec = -19d12'45".9) SN 2003bw is hosted by IC 1077, a face-on spiral galaxy. The new object is superimposed on the western arm. The expected maximum of typical SN Ia is mag about 15.2, though it seems not a case (vsnet-campaign-sn 583). SN 2003cb (RA = 13h00m33s.25, Dec = -06d51'09".3) SN 2003cb is hosted by NGC 4885, apparently disk type galaxy. The expected maximum for typical SN Ia is mag about 15.0, though it seems not to of this case (vsnet-campaign-sn 584). (continuous targets) V982 Oph (RA = 17h52m37s.86, Dec = +07d33'04".4) The outburst was confirmed by K. Torii on March 11 (vsnet-campaign-dn 3530). T. Kato reported that the light curve on March 11 seems to suggest the presence of ~0.2 mag variation, which looks like superhumps with a period of ~0.075 d. There was no rapidly fading trend. Owing to the short visibility and the faintness of the object, the identification of this period is not yet clear (vsnet-campaign-dn 3537). M. Linnolt reported that it was fainter than 15.4 mag on March 12 (vsnet-campaign-dn 3532). AH Her (RA = 16h44m09s.99, Dec = +25d15'02".1) A possible weak outburst can be seen around March 1-3 during the standstill (vsnet-campaign-dn 3529). SN 2003bm (RA = 08h07m22s.87, Dec = +40d23'44".3) A spectrum taken on Mar. 7 by the CfA team revealed that it is type Ic supernova (vsnet-campaign-sn 579). DM Dra (RA = 15h34m12s.13, Dec = +59d48'31".9) Based on March 7-13 data, the best period of superhumps has been determined to be 0.07567(2) d (vsnet-campaign-dn 3531, 3534, 3542). Secondary superhump maxima sometimes appeared on March 10 (vsnet-campaign-dn 3534). The amplitude of the superhumps seems to have quickly decayed during the observation on March 11. On March 13, the full amplitude is reduced to 0.1 mag (vsnet-campaign-dn 3542). The superoutburst continues (vsnet-campaign-dn 3544). V603 Aql (RA = 18h48m54s.6, Dec = +00d35'03") Based on D. West's observations, T. Kato reported that the object looks indeed systematically fainter than the past years, even taking the slow general fading since the nova outburst into account (vsnet-campaign-nova 1171, 1172). SN 2003bp (RA = 08h27m27s.81, Dec = +17d17'14".5) A spectrum taken on Mar. 10 by the CfA team revealed that it is type Ib supernova, but the He line is weaker than normal SN Ib. They suggest that it would be a transitional object between SN Ib and Ic (vsnet-campaign-sn 579). The LBNL team also report that a spectrum taken on Mar 8.22 shows it to be an early SN Ib with somewhat weaker He lines (vsnet-campaign-sn 580). SN 2003br (RA = 14h34m34s.98, Dec = -27d59'48".8) A spectrum taken on Mar 11.47 by the CfA team revealed that it is a type II SN (vsnet-campaign-sn 580). MisV1147 (RA = 22h54m03s.78, Dec = +58d54'02".1) D. West reported a deep fading (>15.3V) of MisV1147 on March 15 (vsnet-campaign-unknown 195). AM Her (RA = 18h16m13s.4, Dec = +49d52'03".1) The brightening may have stopped (vsnet-campaign-polar 23). R CrB (RA = 15h48m34s.40, Dec = +28d09'23".7) After the object reached at minimum, it may start recovering (vsnet-campaign-rcb 111, 112, 113, 114, 115, 116, 117, 118). V2540 Oph (RA = 17h37m34s.36, Dec = -16d23'18".4) D. West reported that V2540 Oph is gradually getting bluer, but T. Kato commented that it is because the contribution from H_alpha emission line has reduced (vsnet-campaign-nova 1169, 1170). *** Future schedule *** The 3rd International Workshop for Comprehensive Study of the High Energy Universe - Toward Very High Energy Particle Astronomy - Date: Mar. 20-22, 2003 Location: ICRR, Univ. of Tokyo, Kashiwa, Japan web site: http://taws300.icrr.u-tokyo.ac.jp/workshop2003/ [vsnet-campaign-blazar 297] eta Car: The next "shell event"/X-ray eclipse M. Corcoran reported the event will occur this summer. Coordinated ground-based observations of eta car along with the X-ray observations would be really important. For more information: Latest X-ray light curve: http://lheawww.gsfc.nasa.gov/users/corcoran/eta_car/etacar_rxte_lightcurve/ [vsnet-campaign-sdor 23, 24, 25, 26, 28, 29] [vsnet-campaign-xray 172] Light curve provided by S. Otero: http://ar.geocities.com/varsao/Curva_Eta_Carinae.htm [vsnet-campaign-sdor 22] The 2003 Gamma Ray Burst conference Hosted by Los Alamos, in Santa Fe, New Mexico (USA), between September 8 and 12, 2003 http://grb2003.lanl.gov/ [vsnet-campaign-grb 13] WEBT campaign on Mkn 421 M. Villata announced possible WEBT campaign on Mkn 421, in December 2002 and February-March 2003, to be carried out during multifrequency campaigns. The relevant information on the MW campaign of December 2-16 is at the VERITAS site <http://veritas.sao.arizona.edu> . [vsnet-campaign-blazar 287] [vsnet-campaign-blazar 288] SUPERNOVAE (10 YEARS OF SN1993J) 22-26 April 2003, Valencia, Spain Web site: http://vsnet.uv.es/2003supernovae/ [vsnet-campaign-sn 342] [vsnet-campaign-sn 452] [vsnet-campaign-sn 512] *** General information *** V982 Oph CCD image taken by K. Torii: http://vsnet.kusastro.kyoto-u.ac.jp/pub/vsnet/DNe/V982_Oph/torii1.gif http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/v982oph.html [vsnet-campaign-dn 3530] GRB 021004 Preprint by M. Uemura et al. http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/GRB/grb021004.html [vsnet-campaign-grb 14] 1RXP J113123+4322.5 VSNET page: http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/j1131.html [vsnet-campaign-dn 3536] Superhump profile: http://vsnet.kusastro.kyoto-u.ac.jp/pub/vsnet/DNe/J1131/j1131-0313.gif [vsnet-campaign-dn 3540] Needs More Observations (NMO) Campaign: http://vsnet.aavso.org/bulletin/ [vsnet-campaign-mira 51, 52] (This summary can be cited.) Regards, Makoto Uemura
vsnet-adm@kusastro.kyoto-u.ac.jp