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ASTROPHYSICS: STUDY RESULTS FROM A.L. GYULBUDAHGIAN ET AL PROVIDE NEW INSIGHTS INTO ASTROPHYSICS
Science Letter
December 16, 2008
"Recent studies of the star formation region BBW 36 and associated
molecular clouds are presented. The (CO)-C-12 (1-0) observations,
carried out with the 15-m SEST (Swedish-ESO) telescope (Cerro La Silla,
Chile), revealed the existence of cloud a, connected with BBW 36 and
of cloud b, having elongation in SE-NW direction," scientists writing
in the journal Astrophysics report (see also Astrophysics).
"A red-shifted molecular outflow with velocity similar to+5 km/s
(with respect to cloud a), having a direction parallel to the line of
sight, was also observed. VLA observations showed the presence of a
source VLA 2 at 3.6 cm with an elongation in the N-S direction. It is
suggested that the VLA 2 source coincides with a dust disc (surrounding
the object BBW 36). The star 3, which is one of the YSOs in the
star-forming region BBW 36 and is connected with a bright comma-like
nebula, can be the source of the molecular outflow. The star 3 has
very high IR colors and is associated with an IRAS point source IRAS
07280-1829, which has IR colors, typical for an IRAS point source,
connected with a water maser. On the 2MASS K image of BBW 36 we can
see the existence of a bright nebula; a group of stars is embedded
in that nebula, and among these stars there are stars with dust discs
(or envelopes)," wrote A.L. Gyulbudahgian and colleagues.
The researchers concluded: "On the 2MASS K image several spiral jets
are also present, some of them with a condensation at the end."
Gyulbudahgian and colleagues published their study in
Astrophysics (STAR-FORMING REGION BBW 36 IN PUPPIS. Astrophysics,
2008;51(3):394-402).
Additional information can be obtained by contacting
A.L. Gyulbudahgian, VA Ambartsumian Byurakan Astrophysics Observ,
Byurakan, Armenia.
The publisher of the journal Astrophysics can be contacted at:
Springer, Plenum Publishers, 233 Spring St., New York, NY 10013, USA.
Science Letter
December 16, 2008
"Recent studies of the star formation region BBW 36 and associated
molecular clouds are presented. The (CO)-C-12 (1-0) observations,
carried out with the 15-m SEST (Swedish-ESO) telescope (Cerro La Silla,
Chile), revealed the existence of cloud a, connected with BBW 36 and
of cloud b, having elongation in SE-NW direction," scientists writing
in the journal Astrophysics report (see also Astrophysics).
"A red-shifted molecular outflow with velocity similar to+5 km/s
(with respect to cloud a), having a direction parallel to the line of
sight, was also observed. VLA observations showed the presence of a
source VLA 2 at 3.6 cm with an elongation in the N-S direction. It is
suggested that the VLA 2 source coincides with a dust disc (surrounding
the object BBW 36). The star 3, which is one of the YSOs in the
star-forming region BBW 36 and is connected with a bright comma-like
nebula, can be the source of the molecular outflow. The star 3 has
very high IR colors and is associated with an IRAS point source IRAS
07280-1829, which has IR colors, typical for an IRAS point source,
connected with a water maser. On the 2MASS K image of BBW 36 we can
see the existence of a bright nebula; a group of stars is embedded
in that nebula, and among these stars there are stars with dust discs
(or envelopes)," wrote A.L. Gyulbudahgian and colleagues.
The researchers concluded: "On the 2MASS K image several spiral jets
are also present, some of them with a condensation at the end."
Gyulbudahgian and colleagues published their study in
Astrophysics (STAR-FORMING REGION BBW 36 IN PUPPIS. Astrophysics,
2008;51(3):394-402).
Additional information can be obtained by contacting
A.L. Gyulbudahgian, VA Ambartsumian Byurakan Astrophysics Observ,
Byurakan, Armenia.
The publisher of the journal Astrophysics can be contacted at:
Springer, Plenum Publishers, 233 Spring St., New York, NY 10013, USA.