Object structure

Ամսագրի կամ հրապարակման վերնագիր:

Բյուրականի աստղադիտարանի հաղորդումներ: Երևանի աստղադիտարանի բյուլետեն = Сообщения Бюраканской обсерватории. Бюллетень ереванской Астрономической обсерватории = Contributions from the Burakan observatory. Bulletin of the Erevan astronomical observatory

Հրապարակման ամսաթիւ:

2020

Հատոր:

67

Համար:

2

ISSN:

2579-2276

Վերնագիր:

Investigation of faint galactic carbon stars from the First Byurakan Spectral Sky Survey. IV. GAIA DR2 data

Ստեղծողը:

Kostandyan, G. R.

Խորագիր:

Astrometry ; Space Sciences ; Archaeoastronomy and Astronomy in Culture

Չվերահսկուող բանալի բառեր:

carbon stars ; surveys ; late - type stars

Ծածկոյթ:

206-210

Ամփոփում:

The second Gaia data release (Gaia DR2) data are used to analyze and estimate a some important parameters for 127 carbon (C) type stars (56 are late N - type Asymptotic Giant Branch (AGB) C stars, 71 are early -type CH giants) detected on the First Byurakan Spectral Sky Survey (FBS) low - resolution (lr) spectral plates. Gaia DR2 G broad band magnitudes are in the range 9.4 mag < G < 18.2 mag. for FBS C stars. Radial velocities (RV) is available for 75 C stars out of 127. For 9 objects RV is greater than 200 km/s. Absolute magnitudes in V band are estimated for 18 FBS C stars, having luminosity data, from which 17 are CH giants. They are in the range between -3.5 ≤ MV < +0.5 mag. For FBS 1918+869 absolute magnitude MV = -3.4(±0.2) mag, which is typical for N type AGB C stars. Having distance estimations, the Hertzsprung - Russell diagram (HRD, or color - absolute magnitude diagram) was constructed for C stars. All FBS detected C stars are giants and AGB stars in the Galactic Halo. They are not far than 14 kpc from the Sun and 8 kpc from the Galactic plane.

Տեսակ:

Հոդված

Ձեւաչափ:

pdf

Լեզու:

en

Գլխաւոր նշումը:

Communications of the Byurakan Astrophysical Observatory (ComBAO) is a peer-reviewed scientific journal, which publishes research in observational and theoretical astronomy/astrophysics and presents recent advances in these fields. It is being published by the NAS RA V. Ambartsumian Byurakan Astrophysical Observatory (BAO) in English in electronic form. The journal publishes original papers, review papers, brief reports, book reviews, special communications, observational and theoretical results in various fields of astronomy and related sciences, and some editorial notes, including anniversaries and obituaries. Under the heading “Legacy”, the renewed magazine will republish some old articles of high value in English. The heading “Guest articles” will bring to the attention of readers the articles of researchers who are not employees of BAO. ComBAO was founded in 1946 and regularly published in 1946-1990. However, the publication was interrupted because of the economic situation after the disintegration of the Soviet Union in 1991.

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