output
19952026
most citedThe UKIRT Infrared Deep Sky Survey (UKIDSS)

2.5k citations

Showing 2017Show all

57 papers · 1 filter

astro-ph.IM2017★ 1 cited

Accurate photometry with digitized photographic plates of the Moscow collection

K. V. Sokolovsky, A. M. Zubareva, D. M. Kolesnikova +3

Photographic plate archives contain a wealth of information about positions and brightness celestial objects had decades ago. Plate digitization is necessary to make this informati…

astro-ph.GA2017★ 9 cited

Relation between parameters of dust and parameters of molecular and atomic gas in extragalactic star-forming regions

K. I. Smirnova, M. S. Murga, D. S. Wiebe +1

The relationships between atomic and molecular hydrogen and dust of various sizes in extragalactic star-forming regions are considered, based on observational data from the Spitzer…

astro-ph.GA2017★ 7 cited

Star-forming complexes in the polar ring galaxy NGC660

K. I. Smirnova, D. S. Wiebe, A. V. Moiseev

Galaxies with polar rings consist of two subsystems, a disk and a ring, which rotate almost in orthogonal planes. In this paper, we analyze the parameters characterizing the compos…

astro-ph.SR2017

Multi-wavelength observations of planet forming disks: Constraints on planet formation processes

Inga Kamp, Stefano Antonellini, Andres Carmona +2

Our understanding of protoplanetary disks has greatly improved over the last decade due to a wealth of data from new facilities. Unbiased dust surveys with Spitzer leave us with go…

astro-ph.SR2017★ 1 cited

Spotted surface structure of the active giant PZ Mon

Yu. V. Pakhomov, K. A. Antonyuk, N. I. Bondar' +3

Based on our photometric observations in 2015-2016 and archival photometric data for the active red giant PZ Mon, we have found the main characteristics of the stellar surface: the…

astro-ph.SR2017★ 82 cited

The close circumstellar environment of Betelgeuse - V. Rotation velocity and molecular envelope properties from ALMA

Pierre Kervella, Leen Decin, Anita M. S. Richards +6

We observed Betelgeuse using ALMA's extended configuration in band 7 (f~340 GHz, λ~0.88 mm), resulting in a very high angular resolution of 18 mas. Using a solid body rotation mode…