PUBBLICAZIONI

Astrophysics and Space Science

An International Journal of Astronomy, Astrophysics and Space Science

ISSN 0004-640X

Astrophys Space Sci

DOI 10.1007/s10509-014-1854-6

February 17, 2014

Asteroids’ physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution

Astronomy & Astrophysics manuscript no. hanus_2013_AA

January 30, 2013

ESO 2013

Photometric analysis of the spin parameters and shapes for the C-type main-belt asteroids (171) Ophelia and (360) Carlova

Astronomy & Astrophysics manuscript no. wang˙Muinonen˙paper1˙KM c ESO 2013

January 24, 2013

ESO 2013

Asteroids’ physical models from combined dense and sparse photometry and scaling of the YORP effect by the  observed obliquity distribution (2012).

Earth and Planetary Astrophysics (astro-ph.EP)

DOI:0.1051/0004-6361/201220701

ESO 2013

Photometry and models of selected main belt asteroids - IX. Introducing interactive service for asteroid models  (ISAM). (2012)

A&A 545, A131 (2012)

DOI: 10.1051/0004-6361/201219542

ESO 2012

Do Slivan states exist in the Flora family? - I. Photometric survey of the Flora region (2012)

A&A 546, A72 (2012)

DOI: 10.1051/0004-6361/201219199

ESO 2012

Electronic Telegram No. 2698 Central Bureau for Astronomical Telegrams (2011)

INTERNATIONAL ASTRONOMICAL UNION

CBAT Director: Daniel W. E. Green; Hoffman Lab 209; Harvard University;

20 Oxford St.; Cambridge, MA 02138; U.S.A.

Electronic Telegram No. 2193 Central Bureau for Astronomical Telegrams (2010)

INTERNATIONAL ASTRONOMICAL UNION

CBAT Director: Daniel W. E. Green; Room 209; Dept. of Earth and Planetary

Sciences; Harvard University; 20 Oxford St.; Cambridge, MA 02138; U.S.A.

Electronic Telegram No. 2193 Central Bureau for Astronomical Telegrams (2010)

INTERNATIONAL ASTRONOMICAL UNION

CBAT Director: Daniel W. E. Green; Room 209; Dept. of Earth and Planetary

Sciences; Harvard University; 20 Oxford St.; Cambridge, MA 02138; U.S.A.

New insights on the binary asteroid 121 Hermione

Based on observations from program 077.C-0422 

collected at the European Southern Observatory, Chile

Discovery of the binary natureof the Mars–crosser (1139) Atami

Astronomy & Astrophysics manuscript no. asters2 c ESO 2008

September 29, 2008

ESO 2008

HD 17156b: A Transiting Planet with a 21.2 Day Period and anEccentric Orbit

Astronomy & Astrophysics manuscript no. mbarbieri 

February 2, 2008

M. Barbieri1, R. Alonso1, G. Laughlin2, J. M. Almenara3, R. Bissinger4, D. Davies5,

ESO 2008

HD 17156b: A Transiting Planet with a 21.2 Day Period and an

Eccentric Orbit

Astronomy & Astrophysics manuscript no. hd17156˙v5

October 3, 2007

ESO 2007

Volume 34, number 4 A.D: 2007 October-December

Lighcurve Analysis of 235 CAROLINA pag.100

Physical models of ten asteroids from an observers’ collaboration network (2007)

A&A 465, 331–337 (2007)

DOI: 10.1051/0004-6361:20066347

ESO 2007

Electronic Telegram No. 464 Central Bureau for Astronomical Telegrams (2006)

INTERNATIONAL ASTRONOMICAL UNION

M.S. 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.

IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions)

CBAT@CFA.HARVARD.EDU (science)

Electronic Telegram No. 430 Central Bureau for Astronomical Telegrams (2006)

INTERNATIONAL ASTRONOMICAL UNION

M.S. 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.

IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions)

CBAT@CFA.HARVARD.EDU (science)

Four new binary minor planets:

(854) Frostia, (1089) Tama, (1313) Berna, (4492) Debussy

A&A 446, 1177–1184 (2006)

DOI: 10.1051/0004-6361:20053709

ESO 2006