58 research outputs found

    The Extragalactic Distance Database: Color-Magnitude Diagrams

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    The CMDs/TRGB (Color-Magnitude Diagrams/Tip of the Red Giant Branch) section of the Extragalactic Distance Database contains a compilation of observations of nearby galaxies from the Hubble Space Telescope. Approximately 250 (and increasing) galaxies in the Local Volume have CMDs and the stellar photometry tables used to produce them available through the web. Various stellar populations that make up a galaxy are visible in the CMDs, but our primary purpose for collecting and analyzing these galaxy images is to measure the TRGB in each. We can estimate the distance to a galaxy by using stars at the TRGB as standard candles. In this paper we describe the process of constructing the CMDs and make the results available to the public.Comment: 8 pages, 5 figures, 1 long table, submitted to Astronomical Journa

    Probe of dark galaxies via disturbed/ lopsided isolated galaxies

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    Searching for lopsided/interacting objects among ~1500 isolated galaxies yields only eight strongly disturbed galaxies which may be explained as a result of their interaction with massive dark objects. We present results of spectral and photometric observations of these galaxies performed with the 6-m telescope that lead to significant restriction on cosmic abundance of dark galaxies.Comment: To appear in proceedings IAU Symp 244, 'Dark Galaxies and Lost Baryons', June 200

    Tip of the Red Giant Branch Distances. I. Optimization of a Maximum Likelihood Algorithm

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    Accurate distances to galaxies can be determined from the luminosities of stars at the Tip of the Red Giant Branch (TRGB). We use a Maximum Likelihood algorithm to locate the TRGB in galaxy color-magnitude diagrams. The algorithm is optimized by introducing reliable photometric errors and a completeness characterization determined with artificial star experiments. The program is extensively tested using Monte-Carlo simulations, artificial galaxies, and a sample of nearby dwarf galaxies observed with HST/WFPC2 and ACS. Our procedure is shown to be reliable, to have good accuracy, and to not introduce any systematic errors. The methodology is especially useful in cases where the TRGB approaches the photometric limit and/or the RGB is poorly populated.Comment: submitted to A

    Lena Delta hydrology and geochemistry: long-term hydrological data and recent field observations

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    The Lena River forms one of the largest deltas in the Arctic. We compare two sets of data to reveal new insights into the hydrological, hydrochemical, and geochemical processes within the delta: (i) long-term hydrometric observations at the Khabarova station at the head of the delta from 1951 to 2005; (ii) field hydrological and geochemical observations carried out within the delta since 2002. Periods with differing relative discharge and intensity of fluvial processes were identified from the long-term record of water and sediment discharge. Ice events during spring melt (high water) reconfigured branch channels and probably influenced sediment transport within the delta. Based on summer field measurements during 2005–2012 of discharge and sediment fluxes along main delta channels, both are increased between the apex and the front of the delta. This increase is to a great extent connected with an additional influx of water from tributaries, as well as an increase of suspended and dissolved material released from the ice complex. Summer concentrations of major ion and biogenic substances along the delta branches are partly explained by water sources within the delta, such as thawing ice complex waters, small Lena River branches and estuarine areas

    Lignite from Central Watershed of the Yenisei River and Prospects for their use for Manufacture of Germanium

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    Π›ΠΈΠ³Π½ΠΈΡ‚Ρ‹ срСднСго тСчСния Ρ€. ЕнисСй, Π»ΠΎΠΊΠ°Π»ΠΈΠ·ΠΎΠ²Π°Π½Π½Ρ‹Π΅ Π² ΠΏΡ€Π΅Π΄Π΅Π»Π°Ρ… мСзокайнозойских ΠΎΡ‚Π»ΠΎΠΆΠ΅Π½ΠΈΠΉ Касской Π²ΠΏΠ°Π΄ΠΈΠ½Ρ‹, Ρ€Π°ΡΡΠΌΠ°Ρ‚Ρ€ΠΈΠ²Π°ΡŽΡ‚ΡΡ ΠΊΠ°ΠΊ Π½ΠΎΠ²Ρ‹ΠΉ пСрспСктивный источник Π³Π΅Ρ€ΠΌΠ°Π½ΠΈΠ΅Π²ΠΎΠ³ΠΎ ΡΡ‹Ρ€ΡŒΡ Π² России. ΠŸΡ€ΠΈΠ²Π΅Π΄Π΅Π½Ρ‹ Ρ€Π΅Π·ΡƒΠ»ΡŒΡ‚Π°Ρ‚Ρ‹ изучСния Ρ„ΠΈΠ·ΠΈΠΊΠΎ-химичСских свойств ΠΈ тСхнологичСских исслСдований, ΠΏΠΎΠ·Π²ΠΎΠ»ΡΡŽΡ‰ΠΈΠ΅ ΠΎΡ†Π΅Π½ΠΈΡ‚ΡŒ Π²ΠΎΠ·ΠΌΠΎΠΆΠ½ΠΎΡΡ‚ΡŒ выдСлСния гСрмания ΠΈΠ· Π»ΠΈΠ³Π½ΠΈΡ‚ΠΎΠ² Π² процСссС ΠΈΡ… сТигания для ΠΎΡ‚Ρ€Π°Π±ΠΎΡ‚ΠΊΠΈ, Π° Π² ΠΏΠΎΡΠ»Π΅Π΄ΡƒΡŽΡ‰Π΅ΠΌ для ΠΏΡ€ΠΎΠΌΡ‹ΡˆΠ»Π΅Π½Π½ΠΎΠΉ Ρ‚Π΅Ρ…Π½ΠΎΠ»ΠΎΠ³ΠΈΠΈ Π΅Π³ΠΎ извлСчСнияLignite from central watershed of the Yenisei river localized within the Meso-Cenozoic cavity deposit considered as a promising new source of germanium raw materials in Russia. Germanium separating possibility from lignite during the combustion process has been studied on the base of physical and chemical properties research in order to develop the industrial technolog

    ACS imaging of 25 galaxies in nearby groups and in the field

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    We present HST/ACS images and color-magnitude diagrams for 25 nearby galaxies with radial velocities V_LG < 500 km/s. Distances are determined based on the luminosities of stars at the tip of the red giant branch that range from 2 Mpc to 12 Mpc. Two of the galaxies, NGC 4163 and IC 4662, are found to be the nearest known representatives of blue compact dwarf (BCD) objects. Using high-quality data on distances and radial velocities of 110 nearby field galaxies, we derive their mean Hubble ratio to be 68 km/(s Mpc) with standard deviation of 15 km/(s Mpc). Peculiar velocities of most of the galaxies, V_pec = V_LG - 68 D, follow a Gaussian distribution with sigma_v = 63 km/s, but with a tail towards high negative values. Our data displays the known correlation between peculiar velocity and galaxy elevation above the Local Supercluster plane. The small observed fraction of galaxies with high peculiar velocities, V_pec < -500 km/s, may be understood as objects associated with nearby groups (Coma I, Eridanus) outside the Local volume.Comment: 17 pages, 8 figures, accepted to A
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