Beiträge von Mark Biesmans im Thema „Aktuelle Schätzungen an sonst. Veränderlichen“

    Observed chi Cyg at magn. 4.6 using comp. stars 44 (theta Lyr) and 47 (phi Cyg).
    Naked eye observation done here in Essen, Belgium at 01 hrs 02 min. (local time) on August 6th.


    Checked chi Cyg and the comp. stars used also with 7x 40 mm binoculars.
    Chi is much brighter than the 47 = phi Cyg and comp. star 44 = theta Lyr is hugely much brighter.
    Those 7x 40 mm binoculars have way too much aperture/light gathering power to make a nice clean observation of chi Cyg.


    To the naked eye I found chi Cyg a tad brighter than the 47 comp. star.
    Comp. star 44 was much easier.
    The magn. 5.0 star (17 Cyg) very close (just to the west) to chi Cyg was also visible to the naked eye.


    All comp. star magnitudes are Hipparcos photometric values.
    Checked the B-V of the comp. stars too.
    The 44 comp. star (theta Lyr) is a bit reddish (B-V 1.26) but OK to use as phi Cyg has a B-V of 0.97 (dark yellow)
    so the difference in B-V of both comp. stars is quite similar/not too far out of range.


    Will send my other observations later today in a complete report.


    Rgds,
    bmm

    Hi Ronny,


    Bin kein Spezialist bez. Fotometrie oder Fotografie.
    Mache nur rein visuelle Beobachtungen.
    Sorry.


    MfG,
    bmm


    <blockquote id="quote"><font size="1" face="Verdana, Arial, Helvetica" id="quote">Zitat:<hr height="1" noshade id="quote"><i>Original erstellt von: nemausa</i>
    <br /><blockquote id="quote"><font size="1" face="Verdana, Arial, Helvetica" id="quote">Zitat:<hr height="1" noshade id="quote">If you or anyone else has a question about variable star observing, I will be glad to answer it.<hr height="1" noshade id="quote"></blockquote id="quote"></font id="quote">
    Hallo Marc,


    ok, da hätte ich gleich mal eine Frage. Ich habe bisher zwar nur wenige Sterne mit höherer Genauigkeit (ca.0,02 mag) fotometriert, aber dabei ist mir etwas aufgefallen. Die bisher gemessenen Roten Riesensterne sind innerhalb weniger Wochen alle leicht veränderlich mit einer Amplitude in der Größenordnung von 0,05 bis 0,2 mag. Auch dann, wenn diese Roten Riesen gar nicht als veränderlich bekannt sind und eigentlich konstant sein sollten, wie beispielsweise HD 283277.


    Gibt es überhaupt konstante Rote Riesensterne?
    Sollte man als Vergleichsstern zur genaueren Fotometrierung grundsätzlich nur Hauptreihensterne und keine Riesensterne verwenden?


    Viele Grüße,
    Ronny
    <hr height="1" noshade id="quote"></blockquote id="quote"></font id="quote">

    Hi Guenther,


    The observing report of the variables I am submitting here, is in fact a copy of my report that I send in to
    the database of VSNet at the University of Kyoto in Japan.
    For years I am making my report that way.
    My main goal is that this report is as informative as possible to myself.
    I started with astronomical observing in 1980 and from april 1994 I only observe variable stars.
    I owned more than 300 telescopes in the past, so with this report I can always check what kind of magnitude I
    could see with what kind of telescope.
    I only use my own charts and sequences as they are way better, beautiful and much more scientifically correct than
    anything else "out there".
    I am an ex AAVSO chartmaker (and for some time also the Chartmaster).
    The variables I like to observe are rather faint, but they are my favorites.
    Besides those, I also regularly observe a list of very unknown Mira stars, most of them don't have even an AAVSO sequence.
    I still have to make a lot of charts and sequences of those unknown Mira stars but they have to wait till more APASS photometry
    becomes available.
    By the way: on July 29. AAVSO announced data release DR9 of APASS.
    Unfortunately after even this 9th release, there are still fields that don't have CCDV photometry.
    It is a real waiting game, that will be over once the GAIA satellite photometry will become availabe next year.
    If you or anyone else has a question about variable star observing, I will be glad to answer it.
    You can write me in English (preferably), German, French or Dutch.


    Best regards,
    Marc

    Observer: Marc Biesmans, Essen, Belgium
    Initials: BMM
    Internet: marcbiesmans(==&gt;)yahoo.com


    Instruments: Celestron C11 XLT: 280 mm f/10 Schmidt-Cassegrain on Astro-Physics AP1100 GTO equatorial mount (SC 280)
    + TS 90 mm f/6.6 apochromatic refractor (R 90)


    All charts and sequences: BMM


    Visual observations for July 26, 2015
    All times: UT


    Date(UT) Star Magn. Comp.stars Chart info Power Aperture Seq. photometry


    LPV's


    20150726.1 And SX 9.6 BMM 94-98 C071211 30 x R 90 TASS-V + CCDV Henden
    20150726.1 Peg RR 9.6 BMM 95-98 C120305 38 x R 90 ASAS-3(V) + CCDV APASS
    20150726.1 Psc W 12.4 BMM 120-125 D100318 175 x SC 280 ASAS-3(V) + CCDV Henden


    Regards,
    Marc

    Observer: Marc Biesmans, Essen, Belgium
    Initials: BMM
    Internet: marcbiesmans(==&gt;)yahoo.com


    Instruments: Celestron C11 XLT: 280 mm f/10 Schmidt-Cassegrain on Astro-Physics AP1100 GTO equatorial mount (SC 280)
    + TS 90 mm f/6.6 apochromatic refractor (R 90)


    All charts and sequences: BMM


    Visual observations for July 19/20, 2015
    All times: UT


    Date(UT) Star Magn. Comp.stars Chart info Power Aperture Seq. photometry


    LPV's


    20150720.0 And RY &lt;14.6 BMM 146 E070710 255 x SC 280 TASS-V + CCDV Henden
    20150720.0 And UW 14.1 BMM 139-143 E091123 215 x SC 280 TASS-V + CCDV Henden
    20150719.9 Aql LO 11.4 BMM 109-115-117 E120225 47 x SC 280 CCDV Zissell
    20150719.9 Aql SY 9.9 BMM 95-100 D090906 25 x R 90 ASAS-3(V) + CCDV Henden
    20150719.9 Aql TV 13.0 BMM 125-130-134 E080510 117 x SC 280 ASAS-3(V) + CCDV Henden
    20150720.0 Cyg DG 13.0 BMM 128-132 E090508 88 x SC 280 TASS-V + CCDV Henden
    20150719.9 Cyg FL 13.9 BMM 134-140 E070520 175 x SC 280 Tycho-2 + CCDV Henden
    20150720.0 Cyg WY &lt;14.4 BMM 144 E080523 255 x SC 280 Tycho-2 + CCDV Henden
    20150720.0 Del RX &lt;14.8 BMM 148 E130330 255 x SC 280 ASAS-3(V) + CCDV APASS
    20150720.0 Del SS &lt;15.1 BMM 151 E050915 311 x SC 280 ASAS-3(V) + CCDV Zissell
    20150720.0 Equ RR 11.9 BMM 118-121 E130610 70 x SC 280 ASAS-3(V) + CCDV APASS
    20150719.9 Her AE &lt;14.2 BMM 142 E080805 255 x SC 280 ASAS-3(V) + CCDV Henden
    20150720.0 Lac W 11.3 BMM 112-114 E071213 30 x R 90 TASS-V + CCDV Henden
    20150719.9 Lyr AN &lt;14.6 BMM 146 E031130 255 x SC 280 TASS-V + CCDV Henden
    20150719.0 Lyr EL &lt;14.6 BMM 146 F120225 255 x SC 280 TASS-V + CCDV Zissell
    20150719.0 Lyr RX &lt;15.0 BMM 150 F090210 255 x SC 280 Tycho-2 + CCDV Henden
    20150719.9 Lyr RY 14.6 BMM 145-148 E090512 255 x SC 280 TASS-V + CCDV Henden
    20150720.0 Peg AN 13.5 BMM 132-136 E130516 117 x SC 280 ASAS-3(V) + CCDV APASS
    20150720.0 Peg DL 13.5 BMM 132-136-138 D080704 117 x SC 280 ASAS-3(V) + CCDV Henden
    20150720.0 Peg TV &lt;14.7 BMM 147 E120621 311 x SC 280 ASAS-3(V) + CCDV APASS


    Regards,
    Marc