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NEAR-CONTACT BINARY V836 Cygni Çanakkale, 2004

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NEAR-CONTACT BINARY V836 Cygni Çanakkale, 2004. Observations. Ege University Obs. (30 cm.) Turkish National Obs. (40 cm.) Date range:2000-2002 U B V filters. No brightness deficiency at 0.5 (Zhukov & Markova1994) but at ~1.1. Before the analysis. Mode definition for WD code - PowerPoint PPT Presentation
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NEAR-CONTACT BINARY NEAR-CONTACT BINARY V836 Cygni V836 Cygni Çanakkale, 2004
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NEAR-CONTACT BINARYNEAR-CONTACT BINARY

V836 CygniV836 CygniÇanakkale, 2004

ObservationsObservations

Ege University Obs. (30 cm.) Turkish National Obs. (40 cm.) Date range:2000-2002 U B V filters

No brightness deficiency at 0.5(Zhukov & Markova1994)but at ~1.1

Before the analysisBefore the analysis

Mode definition for WD code

Evidence for (semi-detached?) configuration

Breinhorst et al.(1989): “detached, but...”

f2=0.98 ±0.02

Ωcr=2.5911 > f2= 1.0008

f1= 0.9143

*f(m) : Durbeck & Schumann (1982)

NCB test: the criteriaNCB test: the criteria

P < 1 day Facing surfaces < 0.1 orb. radius apart X Not in contact 1 component at or near its Roche lobe Hotter: A v F ; cooler: 1 v 2 later -------------------------------------------------------------- Agreement in M-R-L relations of [Hilditch etal.(1988)] Two comp. lines parallel to the ZAMS [Oh et al. (2000)]

? Harmony in M-R-L relations of collected data

Shaw (1994)

1 2

NCB A

W X x

NCB A

W X

Classification for 836 Classification for 836

NCBs

V1010 Oph FO VirUndermassive

1st:.at or near its R.L. .normal sized

2nd:.inside R.L. .”oversized”

(1-1.5 times) .Max I > Max II

1st:.inside R.L. .normal sized

2nd:. at or near its R.L .”oversized”

(2-3 times) . No Max I > Max II

1st:. at or near its R.L. .”undermassive”2nd:. inside R.L.

.”undermassive” (1-1.5 times)

Marginal contacteg.Hillditch et al. (1988)

Detached ?eg.Hillditch et al. (1988)

Shaw (1994)

about Evolutionabout Evolution

Disadvantage: Single-lined, only f(m) FO Vir type

A. if

come close enough to transfer required energy from hot to cool, photospere of the cool comp. is getting hot

thenA-type W UMa system. Shaw (1994)

!!(AML by magnetic breaking is needed)

B. Longer-period detached systemvia Case-A mass transfer

semi-detached (836 is here)

marginal contact (not in thermal eq.)

the deeper contact A-type W UMa system[Hilditch etal.(1988), Budding(1984)]

1 2

NCB A

W X x

Problems and FutureProblems and Future

Single-lined spectrae. Prevent the morphology from varying study to study, by

reducing the errors. Eg. q range:

q=0.348 Ω cr=2.5699 near R.L.

q=0.358 (10) Ω cr=2.5911 at R.L.

q=0.368 Ω cr=2.6120 at R.L.

AML: “ The secondaries of FO Vir types must be undermassive”.


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