|
BeSS report – June 2012 |
|
·
100 spectra acquired ·
49 objects observed ·
11 observers contributed The highest number
of spectra was submitted by Stephane Ubaud with 28 spectra, André Favaro
observed the highest number of different objects, 19 different Be star. The most observed
objects were del Sco, Shelyak and QR Vul |
Objects observed
|
12
Vul |
HL
Lib* |
20
Vul |
25
Cyg |
25
Vul |
28
Cyg |
31 Peg * |
4 Aql |
4
Her |
|
48
Lib |
59
Cyg |
64
Ser |
66 Oph* |
chi Oph |
CX
Dra* |
del
Sco* |
eps
Cas |
EW
Lac* |
|
FF Cam* |
HD 112028 |
HD 127617 |
HD 162428 |
HD 168135 |
HD 168957* |
HD 169033 |
HD 174105* |
HD 208682 |
|
HL Lib* |
iot Lyr* |
kap Aql |
kap Dra |
lam Cyg* |
nu Cyg |
PHECDA |
pi Aqr |
QR Vul* |
|
SHELIAK |
tet CrB* |
ups Cyg |
ups Sgr* |
V1040 Sco |
V1075 Sco* |
V1294 Aql* |
V1339 Aql*
|
V4031 Sgr |
|
16 Peg |
25 Peg* |
V532 Lyr |
V923 Aql |
zet Oph |
|
|
|
|
Noticeable evolutions of
H-alpha line
|
HD168957 No more emission in H-alpha line
|
CX Dra H-alpha VR peaks are symmetric – in oct 2011 the V/R
seems to have evolved in few months
|
|
Iot Lyr The H-alpha line start to exhibit emission
|
|
Moderate evolutions of H-alpha
line
|
HL Lib V/R variations
|
FF Cam Intensity and V/R
evolutions
|
|
V1075 Sco Intensity decrease
|
HD 174105 Intensity increase
|
|
V1339 Aql Intensity increase
|
V1294 Aql Intensity increase
|
|
V923 Aql variation of V/R H-alpha peaks
|
EW lac variations of V/R H-alpha peaks
|
To continue to monitor
|
Lam Cyg |
QR Vul |
Ups Sgr |
Del Sco |
Objects quite but has evolved in the past
|
Tet CrB
|
25 Peg
|
