... Near-IR broad-band imaging of V1318 Cygni reveals the presence of two distinct stellar components oriented north-south, a result recently reported by Aspin et al. ... The distribution of the high density molecular gas traced by the CS J emission is highly concentrated around V1318 and V1686 Cygni, while the total column density of gas traced by the J shows a ridge morphology centered on these sources. ... A molecular outflow has been detected in CO J . ...

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• NIR Inages of H2O Masers (Abstract)
• G35.20-1.74 (Abstract)
• S155 (Abstract)

... We present the results of ATCA HI line and 20-cm radio continuum observations of the galaxy Quartet NGC 6845. The HI emission extends over all four galaxies but can only be associated clearly with the two spiral galaxies, NGC 6845A and B, which show signs of strong tidal interaction. We derive a total HI mass of 1.8 x 10 10 Msun, most of which is associated with NGC 6845A, the largest galaxy of the group. ... Figure 2: A new galaxy in the NGC6845 galaxy group. ...

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• The galaxy IC 2554
• Programme - Abstract
• SEST -- MOPRA Comparison at Millimetre-Waves

... For this paper: postscript PPEUC CMB index 1 Introduction.. ... We report on a 16 ks X-ray observation with the ROSAT PSPC towards the center of a CMB decrement detected by Jones et al. (1997) in the direction of the quasar pair PC1643+4631 A & B. At the position of the decrement we find no evidence for emission by hot gas which could give rise to the Sunyaev-Zel'dovich effect. ... We conclude that the CMB decrement is not a typical galaxy cluster. ... 2 The ROSAT PSPC observation . ...

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• Exploring the engines of molecular outflows
• Sub-mm and radio observations of water maser sources
• Bojan Nikolic -- 90 GHz Continuum Observations of Messier 66

SMOV still under way, but science observations being made. ... In addition, a subset of the cluster was targeted for deep HST observations with ACS and NICMOS in Cycle 13, while WFPC2 was used recently to search for evidence for disks and jets among the lower-mass memebrs. ... The present observations build on the Cycle 13 program by providing second-epoch data that will allow separation of cluster and field to apparent magnitudes that correspond to masses as low as 3 M Jupiter for cluster members. ...

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• Spitzer Observations of NGC 2547: The Disk Population at 25 Million Years
• LABOCA observations of giant molecular clouds in the southwest region of the
• The Spitzer discovery of a galaxy with infrared emission solely due to AGN

... OCR by H.Andernach 1/96, to be proof-read) This is the first of a series of papers presenting results of a 10-GHz radio continuum survey of the galactic plane region using the 45-m telescope at Nobeyama. ... Weak Nonthermal Sources: A comparison with the Bonn S-GHz survey reveals a number of weak nonthermal sources near the galactic plane. ... For this reason we conducted a survey of the galactic plane region at 10 GHz using the 45-m radio telescope at the Nobeyama Radio Observatory (NRO). ...

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• A fast-scan extragalactic source survey at 4.755 GHz
• A CS and NH3 Survey
• A 20 cm VLA survey of Abell clusters of galaxies

We review the evidence, from rotational modulation, for association of plages and spots on active binaries. ... There is a similar lack of evidence for BY Dra systems. The results can be interpreted as evidence for: (a) the presence of active longitudes which persist on some RS CVn stars for several years, (b) high filling factors in MgII emission and (c) lower filling factors, and therefore greater contrast, in SWP emission. ...

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• Armagh Observatory
• Abstract 203
• Abstract 193

T1650 2002-Jan-28 13:31:52 Technical Page Proposal Type: Regular General Category: Terrestrial Aeronomy Sub-Category: Radar Observation Category: Galactic Total Time Requested: 20 Hours Proposal Title: Observation of the Ulysses/Galileo Dust stream at 1 AU ABSTRACT: We propose to observe and study, utilizing the 430 MHz Arecibo radar, the micrometeor ux associated with the interstellar dust stream detected by the Ulysses and Galileo spacecraft. ... Maybe Part of the observing run. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/HaynestagA2752tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/DarlingtagA1585tp.ps
• http://www.naic.edu/vscience/schedule/tpfiles/ArayatagA2933tp.pdf

... Previous: Generalized Linear Multi-Frequency Imaging in VLBI . ... At Astronomical Observatory of Valencia University (OAUV), CCD observations of asteroids and big planets satellites are obtained since 2001 with a big format camera and several telescopes. ... Software for comparison of single and overlapped CCD fields obtained at different epochs has been developed. ... After images measurement in CCD field, catalogue stars are identified and adjusted with images. ...

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• Distributed Software for Observations in the Near Infrared
• Simulated AXAF Observations with MARX
• The HST Science Data Archive as a Discovery Tool: First Experiment

ROSAT OBSERVATIONS OF PSR 0355+54 and PSR 1642--03 1 Patrick Slane Harvard­Smithsonian Center for Astrophysics 60 Garden Street, Cambridge, MA 02138 USA ABSTRACT PSR 0355+54 and PSR 1642--03 are both radio pulsars whose X­ray behavior was left unresolved by Einstein observations. 1;2 In each case, faint emission was detected near the sources, but appeared to be concentrated 1--2 arcmin from the known pulsar positions. ... Seward, F. D., & Wang, Z­R 1988, ApJ, 332, 199 3. ... 1993, ApJ, 413, L27 7. ...

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• X--ray Activity and PMS Stars.
• Pat Slane: Pulsar Papers
• SAO Summer Intern Program Projects, 2004

... One striking feature is a small source of almost pure H 2 line emission, which is located near one of the compact sources in Orion reported by O'Dell and collaborators (HST-18 = 203-504). ... H-H objects, Proplyds, Orion Bar, H 2 . ... We obtained a series of images across the bright rim of the Orion Bar near the peaks of mm-wave molecular line emission with NICMOS cameras 1-3 (NIC1, NIC2, NIC3) in several filters on 1998 February 18. ... The suggestion of an H-H object does not seem compelling. ...

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• STScI NICMOS Software
• The Evolution of Stars seen with ISOCAM - the Need for NICMOS and VLT Follow...
• A Color Analysis of NICMOS Parallel Observations

... The ROSAT Bright Survey: II. Catalogue of all high-galactic latitude RASS sources with PSPC countrate CR > 0.2 s -1 . ... 1S We present a summary of an identification program of the more than 2000 X-ray sources detected during the ROSAT All-Sky Survey (Voges et al. 1999) at high galactic latitude, |b| > 30degr , with countrate above 0.2 s -1 . This program, termed the ROSAT Bright Survey RBS, is to more than 99.5% complete. ...

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• Публикации
• High-resolution Near-infrared Study of the Deeply Embedded Young Stellar Object
• Binary speckle measurements at Calar Alto. I. (Docobo+, 2001)

... 28.11.2001 . ... Credit: Greg Bacon ( STScI /AVL) Explanation: By directly detecting the atmosphere of a planet outside our Solar System , humanity has taken another small step toward finding extraterrestrial life . ... November 2001 . ... 2001 2002 . ... NASA Web Site Statements, Warnings, and Disclaimers . NASA Official: Jay Norris. ... Publications with keywords: extrasolar planet . Publications with words: extrasolar planet . ... Atmospheres Detected on Two Extrasolar Planets . ...

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• Астронет > Extra Solar Planetary Atmosphere Detected
• Hot Gas Halo Detected Around Galaxy NGC 4631
• Atmospheres Detected on Two Extrasolar Planets

SN 1989B Light Curve Analysis. ... In the light curve depicting their observations, definite trends are noted, here is a "thumb-nail" analysis of the the magnitude estimations of the bright SN (1989B) in the galaxy NGC 3627 (M66). ... The observations were inserted against the V magnitude templete of BL, CCD photometric data, (Wells et. al, (1994) and a color trend (B-V) histogram of the mean type Ia SN (BL)(nutemp.gif). Key Words: Amateur Observations, Supernova, Magnitude Estimates, 1989B . ...

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• An Observational Program to detect Supernovae in the Virgo Cluster.
• APOD: 2001 July 25 - Hot Gas Halo Detected Around Galaxy NGC 4631
• APOD: 2007 February 27 - Atmospheres Detected on Two Extrasolar Planets

... 322, P L21-L24 (1997). Abstract . ... 322, P L25-L28 (1997). ... 322, P L29-L32 (1997). ... 322, P L33-L36 (1997). ... 322, P L37-L40 (1997). ... 322, P L41-L44 (1997). ... 322, P 709-718 (1997). ... 322, P 719-729 (1997). ... 322, P 730-746 (1997). ... 322, P 747-750 (1997). ... 322, P 751-755 (1997). ... 322, P 756-763 (1997). ... 322, P 764-777 (1997). ... 322, P 778-784 (1997). ... 322, P 785-800 (1997). ... 322, P 801-806 (1997). ... 322, P 807-816 (1997). ... helpdesk@link.springer.de . ...

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• Springer LINK:A&A-EE: Table of Contents Volume 317 Number 2 (1997)
• Springer LINK:A&A-EE: Table of Contents Volume 319 Number 1 (1997)
• Springer LINK:A&A-EE: Table of Contents Volume 319 Number 2 (1997)

ASTRONOMICHESKII TSIRKULYAR No.1573, 2010 April 12 1995 2009 . A Comparison of the Latitudinal Variations of the Methane Absorption Bands on Saturn's Disk at Equinoxes 1995 and 2009 Abstract. The observations of Saturn at last equinox 2009 have detected significant differences of the latitudinal variations of the methane absorption from observed at 1995 equinox . ... 1995 . 2008- 2009 , ­ . ... 4 ( 580-880 ) , (.1) , 2008-2009 . ... 2 , 4 725 1995 2009 . ... 1995 2009 15 , 1980 1995 . ...

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• http://comet.sai.msu.ru/~gmr/poster_1.072.pdf
• Multiwavelength Study of Mira Ceti-Type Variable Stars
• Molecular Masers

To appear in "Fourth Workshop on Robotic Autonomous Observatories (2015)"RevMexAA(SC) METEOR OBSERVATIONS WITH MINI-MEGATORTORA WIDE-FIELD MONITORING SYSTEM S. Karpov, 1, 3 N. Orekhova2 G. Beskin, 1, 3 A. Biryukov3,4 S. Bondar,2 E. Ivanov,2 E. Katkova,2 A. Perkov, and V. Sasyuk3 RESUMEN 2 Favor de prop orcionar un resumen en espanol. ... The faintest detected meteors has the peak brightness about 10 mag, while the ma jority - from 4 to 8 mag. ... 2010; Karpov et al. 2013; Beskin et al. ...

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... In the light curve depicting their observations, definite trends are noted, here is a "thumb-nail" analysis of the the magnitude estimations of the bright SN (1989B) in the galaxy NGC 3627 (M66). ... 10 (IAUC # 4742) 2/25 13.3 16 j 2/27 13.5(*) 18 lc 2/28 13.8 19 p 3/1 13.2 20 w 3/2 13.5 21 a 3/4 13.8 23 p 3/6 13.3 25 c 3/7 13.3 26 c 3/8 14.1 27 m 3/8 13.3 27 r 3/9 13.4 28 c 3/9 14.1 28 m 3/10 13.6 29 j 3/10 14.0 29 a 3/11 13.6 30 c 3/11 13.5 30 r 3/11 13.7 30 s 3/13 [13.69 CCD Mag.] ...

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... The task accepts two sources lists: the observation source list and the exposure source list. ... List of selected sources. This le contains a table, called SRCLIST, with the following columns: Name Type Description SRC NUM Integer Source ID from observation source list RA Double RA from exposure source list DEC Double Declination from expoure source list RATE Real Count rate from observation source list COUNTS Real Number of source counts, from exposure source ...

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• http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0050-1-0.ps.gz
• http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0050-1-1.ps.gz
• Home Page

... Observing . ... Solar Observing . ... April 3 (SUN) - Solar Observing, Central Park , Manhattan . ... APRIL'S SKY . ... Lecture Series at the American Museum of Natural History The Amateur Astronomers Association is proud to present an astronomy lecture series from October through May each year for our members and the .. ... The€аAmateur Astronomers Association of New York€аwas organized in 1927 to promote the study of Astronomy, emphasizing its cultural and inspirational value. ...

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• Astro Answers ? The Big Bang, Inflation, and Latest Results from BICEP2 ?
• Lecture Series 2015-2016 ? Amateur Astronomers Association of New York
• Lecture Series 2011-2012 ? тАЬSearching for Earthlike WorldsтАЭ ? Debra Fischer

Young Stars Near Earth: Progress and Prospects ASP Conference Series, Vol. ... A systematic search for new members of this Capricornius association has yielded four new prob­ able members, which we use to derive an age of 5--10 Myr for the group as a whole. ... Capricornius association. ... Discussion and Conclusions In these proceedings we have argued that HD 199143 and HD 358623 are part of a larger group of young stars, which we tentatively name the Capricornius association. ...

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• ESO - Thesis Topic: ALMACAL: the evolution of the molecular gas in galaxies
• Infrared jitter imaging data reduction algorithms
• ESO - Thesis Topic: Foreground emission and Cosmic Microwave background